This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.83 01:45:57.46 +49:08:31.1
132.02655 -12.76464 galactic And Second-epoch detections are separated by 1.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357435910044195712 | 01:45:58.14 +49:08:34.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 57.46 +49 08 31.1 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357435910044195712,2461093.6803,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357435910044195712 20260222.1803 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:57.46 +49:08:31.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.94 01:42:50.83 +43:56:33.5
132.62482 -17.95942 galactic And Second-epoch detections are separated by 2.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350180988727240832 | 01:42:51.82 +43:56:38.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 50.83 +43 56 33.5 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350180988727240832,2461093.6803,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350180988727240832 20260222.1803 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:50.83 +43:56:33.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.49 01:42:04.22 +48:01:55.3
131.61755 -13.98400 galactic And Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.5224+48.0287 | 01:42:03.33 +48:01:57.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 04.22 +48 01 55.3 10.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.5224+48.0287,2461093.6803,10.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.5224+48.0287 20260222.1803 10.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:04.22 +48:01:55.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.38 01:37:53.07 +50:36:24.1
130.42442 -11.58813 galactic And Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405856271827519488 | 01:37:54.20 +50:36:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1952CoRut..32....1H BD+49 422
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 37 53.07 +50 36 24.1 10.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405856271827519488,2461093.6803,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405856271827519488 20260222.1803 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:37:53.07 +50:36:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 31.97 +50 29 42.3 10.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405802666339748096,2461093.6803,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405802666339748096 20260222.1803 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:31.97 +50:29:42.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.36 01:44:36.44 +41:10:50.4
133.58448 -20.58869 galactic And Second-epoch detections are separated by 2.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347624383674439680 | 01:44:36.85 +41:10:54.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 36.44 +41 10 50.4 10.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347624383674439680,2461093.6803,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347624383674439680 20260222.1803 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:36.44 +41:10:50.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.43 01:39:19.25 +49:36:17.6
130.84633 -12.52963 galactic And Second-epoch detections are separated by 7.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405650697513155072 | 01:39:20.05 +49:36:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 19.25 +49 36 17.6 10.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405650697513155072,2461093.6803,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405650697513155072 20260222.1803 10.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:19.25 +49:36:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.65 01:40:52.67 +50:18:02.5
130.96121 -11.79870 galactic And Second-epoch detections are separated by 4.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405785215888892928 | 01:40:54.28 +50:18:01.2 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: K2 1952CoRut..32....1H BD+49 436
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 52.67 +50 18 02.5 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405785215888892928,2461093.6803,10.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405785215888892928 20260222.1803 10.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:52.67 +50:18:02.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.80 01:38:04.85 +49:25:59.4
130.67658 -12.73591 galactic And Second-epoch detections are separated by 2.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.5244+49.4417 | 01:38:05.50 +49:25:58.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1952CoRut..32....1H BD+48 488
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 04.85 +49 25 59.4 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.5244+49.4417,2461093.6803,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.5244+49.4417 20260222.1803 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:04.85 +49:25:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.83 01:38:22.85 +49:17:20.3
130.75317 -12.86858 galactic And Second-epoch detections are separated by 3.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405616337774705280 | 01:38:23.48 +49:17:19.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 22.85 +49 17 20.3 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405616337774705280,2461093.6803,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405616337774705280 20260222.1803 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:22.85 +49:17:20.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.89 01:45:30.58 +49:51:02.0
131.79859 -12.08801 galactic And Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405517244289652224 | 01:45:31.61 +49:51:00.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 30.58 +49 51 02.0 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405517244289652224,2461093.6803,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405517244289652224 20260222.1803 10.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:30.58 +49:51:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.11 01:39:41.54 +49:00:13.9
131.02444 -13.10819 galactic And Second-epoch detections are separated by 1.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405421174461927552 | 01:39:42.24 +49:00:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 41.54 +49 00 13.9 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405421174461927552,2461093.6803,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405421174461927552 20260222.1803 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:41.54 +49:00:13.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.15 01:40:40.90 +50:16:46.3
130.93401 -11.82555 galactic And Second-epoch detections are separated by 0.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405784936714759040 | 01:40:41.87 +50:16:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 40.90 +50 16 46.3 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405784936714759040,2461093.6803,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405784936714759040 20260222.1803 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:40.90 +50:16:46.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.24 01:40:24.74 +49:45:59.4
130.99214 -12.33725 galactic And Second-epoch detections are separated by 0.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405558957012659200 | 01:40:25.50 +49:45:58.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 24.74 +49 45 59.4 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405558957012659200,2461093.6803,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405558957012659200 20260222.1803 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:24.74 +49:45:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.20 01:40:39.39 +45:07:34.2
131.97220 -16.87988 galactic And Second-epoch detections are separated by 3.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350500220759383040 | 01:40:40.37 +45:07:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 39.39 +45 07 34.2 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350500220759383040,2461093.6803,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350500220759383040 20260222.1803 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:39.39 +45:07:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.24 01:39:55.75 +46:38:07.0
131.53497 -15.42487 galactic And Second-epoch detections are separated by 4.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351094266276417792 | 01:39:56.38 +46:38:09.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 55.75 +46 38 07.0 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351094266276417792,2461093.6803,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351094266276417792 20260222.1803 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:55.75 +46:38:07.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.26 01:40:43.59 +50:37:31.8
130.87268 -11.48475 galactic And Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405798714969830400 | 01:40:44.31 +50:37:28.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 43.59 +50 37 31.8 11.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405798714969830400,2461093.6803,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405798714969830400 20260222.1803 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:43.59 +50:37:31.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.30 01:41:14.46 +46:52:03.6
131.71608 -15.15289 galactic And Second-epoch detections are separated by 6.3" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351123300255342336 | 01:41:15.48 +46:52:08.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 14.46 +46 52 03.6 11.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351123300255342336,2461093.6803,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351123300255342336 20260222.1803 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:14.46 +46:52:03.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.34 01:39:50.16 +50:35:55.4
130.73645 -11.53817 galactic And Second-epoch detections are separated by 3.1" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405809095906985472 | 01:39:51.24 +50:35:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 50.16 +50 35 55.4 11.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405809095906985472,2461093.6803,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405809095906985472 20260222.1803 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:50.16 +50:35:55.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 21.07 +50 27 44.5 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.6803,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260222.1803 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:21.07 +50:27:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.64 01:37:49.92 +50:22:14.3
130.46011 -11.82173 galactic And Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405825863459166080 | 01:37:50.83 +50:22:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 37 49.92 +50 22 14.3 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405825863459166080,2461093.6803,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405825863459166080 20260222.1803 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:37:49.92 +50:22:14.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.71 01:44:15.38 +42:56:25.3
133.11175 -18.88493 galactic And Second-epoch detections are separated by 5.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347887063873678336 | 01:44:16.17 +42:56:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 15.38 +42 56 25.3 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347887063873678336,2461093.6803,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347887063873678336 20260222.1803 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:15.38 +42:56:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.01 01:45:27.42 +50:12:18.1
131.71315 -11.74343 galactic And Second-epoch detections are separated by 6.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405914786462763392 | 01:45:28.74 +50:12:15.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 27.42 +50 12 18.1 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405914786462763392,2461093.6803,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405914786462763392 20260222.1803 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:27.42 +50:12:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.09 02:25:53.93 +46:25:30.0
139.42250 -13.40010 galactic And Second-epoch detections are separated by 0.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 353706607120484608 | 02:25:53.33 +46:25:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 25 53.93 +46 25 30.0 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 353706607120484608,2461093.6803,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 353706607120484608 20260222.1803 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:25:53.93 +46:25:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.03 01:40:36.95 +50:47:45.7
130.82148 -11.32084 galactic Per Second-epoch detections are separated by 1.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406187018669459456 | 01:40:37.98 +50:47:42.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A9V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 36.95 +50 47 45.7 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406187018669459456,2461093.6803,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406187018669459456 20260222.1803 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:36.95 +50:47:45.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.18 01:40:05.55 +50:08:11.8
130.86764 -11.98396 galactic And Second-epoch detections are separated by 3.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405761713827883648 | 01:40:06.62 +50:08:09.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 05.55 +50 08 11.8 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405761713827883648,2461093.6803,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405761713827883648 20260222.1803 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:05.55 +50:08:11.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 11 02.76 +48 56 44.2 8.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RV And,2461093.6803,8.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RV And 20260222.1803 8.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:11:02.76 +48:56:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 32 53.71 +48 20 16.8 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 02399-00354,2461093.6803,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 02399-00354 20260222.1803 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:32:53.71 +48:20:16.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 52 22.70 +48 39 52.3 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Dauban V253,2461093.6803,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Dauban V253 20260222.1803 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:52:22.70 +48:39:52.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 35 51.44 +49 18 00.8 11.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0762 And,2461093.6803,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0762 And 20260222.1803 11.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:35:51.44 +49:18:00.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 32 46.05 +46 29 20.8 8.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
AX And,2461093.6803,8.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AX And 20260222.1803 8.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:32:46.05 +46:29:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.39 01:43:14.67 +42:13:52.2
133.07925 -19.61753 galactic And Second-epoch detections are separated by 2.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.8171+42.2343 | 01:43:14.67 +42:13:52.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 14.67 +42 13 52.2 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.8171+42.2343,2461093.6803,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.8171+42.2343 20260222.1803 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:14.67 +42:13:52.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 31.65 +41 51 38.2 14.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:31.65 +41:51:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.27 01:45:30.78 +41:03:37.4
133.79058 -20.66840 galactic And Second-epoch detections are separated by 8.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.3770+41.0630 | 01:45:30.78 +41:03:37.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 30.78 +41 03 37.4 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.3770+41.0630,2461093.6803,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.3770+41.0630 20260222.1803 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:30.78 +41:03:37.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 48.85 +41 56 55.0 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:48.85 +41:56:55.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 49 01.06 +41 15 55.0 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:49:01.06 +41:15:55.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 49.63 +49 57 37.9 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J014450.26+495736.1,2461093.6803,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J014450.26+495736.1 20260222.1803 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:49.63 +49:57:37.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 11.64 +48 17 05.0 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 592,2461093.6803,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 592 20260222.1803 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:11.64 +48:17:05.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 15.75 +46 40 34.7 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:15.75 +46:40:34.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.13 01:43:31.36 +49:36:07.3
131.53041 -12.39817 galactic And Second-epoch detections are separated by 6.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.8818+49.5990 | 01:43:31.36 +49:36:07.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 31.36 +49 36 07.3 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.8818+49.5990,2461093.6803,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.8818+49.5990 20260222.1803 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:31.36 +49:36:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 38 12.61 +47 05 58.4 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:38:12.61 +47:05:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.95 01:41:50.52 +48:08:44.5
131.55558 -13.88028 galactic And Second-epoch detections are separated by 4.6" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.4570+48.1470 | 01:41:50.52 +48:08:44.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 50.52 +48 08 44.5 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.4570+48.1470,2461093.6803,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.4570+48.1470 20260222.1803 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:50.52 +48:08:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 53.39 +43 50 02.8 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:53.39 +43:50:02.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 10.89 +50 35 07.3 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:10.89 +50:35:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 16.72 +42 18 43.8 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347752786016402560,2461093.6803,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347752786016402560 20260222.1803 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:16.72 +42:18:43.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 07.54 +48 37 06.8 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:07.54 +48:37:06.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 37.26 +44 07 56.8 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:37.26 +44:07:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.91 01:48:15.53 +41:20:03.0
134.26095 -20.28425 galactic And Second-epoch detections are separated by 6.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J027.0702+41.3349 | 01:48:15.53 +41:20:03.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 15.53 +41 20 03.0 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J027.0702+41.3349,2461093.6803,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J027.0702+41.3349 20260222.1803 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:15.53 +41:20:03.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.96 01:41:24.74 +44:25:45.4
132.25573 -17.53585 galactic And Second-epoch detections are separated by 8.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350258293840926848 | 01:41:24.17 +44:25:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 24.74 +44 25 45.4 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350258293840926848,2461093.6803,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350258293840926848 20260222.1803 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:24.74 +44:25:45.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 17.19 +45 40 57.6 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:17.19 +45:40:57.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 29.42 +41 01 54.5 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:29.42 +41:01:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 49 44.56 +49 53 47.1 14.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357863929305526912,2461093.6803,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357863929305526912 20260222.1803 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:49:44.56 +49:53:47.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.97 01:46:33.45 +43:54:35.7
133.31782 -17.84746 galactic And Second-epoch detections are separated by 2.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 349443727523072512 | 01:46:34.23 +43:54:36.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 33.45 +43 54 35.7 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 349443727523072512,2461093.6803,13.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 349443727523072512 20260222.1803 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:33.45 +43:54:35.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 52 40.28 +41 27 03.3 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:52:40.28 +41:27:03.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.75 01:43:45.28 +43:49:24.3
132.81925 -18.04165 galactic And Second-epoch detections are separated by 5.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.9409+43.8239 | 01:43:45.28 +43:49:24.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: A7V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 45.28 +43 49 24.3 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.9409+43.8239,2461093.6803,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.9409+43.8239 20260222.1803 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:45.28 +43:49:24.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.81 01:42:36.23 +48:56:29.8
131.51797 -13.07527 galactic And Second-epoch detections are separated by 5.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405380660031703168 | 01:42:35.01 +48:56:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 36.23 +48 56 29.8 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405380660031703168,2461093.6803,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405380660031703168 20260222.1803 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:36.23 +48:56:29.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 59.66 +48 12 09.0 13.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357333582446334720,2461093.6803,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357333582446334720 20260222.1803 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:59.66 +48:12:09.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.70 01:44:25.79 +43:43:51.0
132.96526 -18.10612 galactic And Second-epoch detections are separated by 8.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.1139+43.7330 | 01:44:25.79 +43:43:51.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 25.79 +43 43 51.0 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.1139+43.7330,2461093.6803,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.1139+43.7330 20260222.1803 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:25.79 +43:43:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.87 01:47:04.56 +47:43:42.6
132.52922 -14.10377 galactic And Second-epoch detections are separated by 4.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:47:04.56 +47:43:42.6 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 04.56 +47 43 42.6 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:04.56 +47:43:42.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.77 01:45:11.31 +49:00:15.4
131.93050 -12.92606 galactic And Second-epoch detections are separated by 8.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357428243525044352 | 01:45:10.64 +49:00:14.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 11.31 +49 00 15.4 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357428243525044352,2461093.6803,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357428243525044352 20260222.1803 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:11.31 +49:00:15.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.80 01:44:14.23 +47:19:45.0
132.13492 -14.59691 galactic And Second-epoch detections are separated by 7.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351175080380516224 | 01:44:14.83 +47:19:43.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 14.23 +47 19 45.0 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351175080380516224,2461093.6803,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351175080380516224 20260222.1803 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:14.23 +47:19:45.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 49 57.88 +49 25 13.3 13.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:49:57.88 +49:25:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.87 01:47:23.85 +49:04:34.6
132.27703 -12.77743 galactic And Second-epoch detections are separated by 7.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.8460+49.0763 | 01:47:23.85 +49:04:34.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 23.85 +49 04 34.6 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.8460+49.0763,2461093.6803,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.8460+49.0763 20260222.1803 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:23.85 +49:04:34.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.77 01:43:17.24 +44:50:12.7
132.50999 -17.06845 galactic And Second-epoch detections are separated by 5.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350372303750248960 | 01:43:18.17 +44:50:09.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 17.24 +44 50 12.7 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350372303750248960,2461093.6803,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350372303750248960 20260222.1803 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:17.24 +44:50:12.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.70 01:49:28.57 +41:36:46.3
134.42724 -19.95977 galactic And Second-epoch detections are separated by 8.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:49:28.57 +41:36:46.3 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 49 28.57 +41 36 46.3 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:49:28.57 +41:36:46.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 13 12.76 +49 57 24.7 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:13:12.76 +49:57:24.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.75 01:47:12.50 +42:46:55.2
133.70638 -18.91995 galactic And Second-epoch detections are separated by 5.6" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:47:12.50 +42:46:55.2 (user input) | T | P | (position from user input) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 12.50 +42 46 55.2 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:12.50 +42:46:55.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.65 01:42:08.85 +48:05:07.3
131.61951 -13.92916 galactic And Second-epoch detections are separated by 8.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399317987275843584 | 01:42:08.24 +48:05:08.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 08.85 +48 05 07.3 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399317987275843584,2461093.6803,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399317987275843584 20260222.1803 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:08.85 +48:05:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.66 01:39:05.41 +49:30:51.1
130.82622 -12.62575 galactic And Second-epoch detections are separated by 8.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.7783+49.5160 | 01:39:04.88 +49:30:57.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 05.41 +49 30 51.1 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.7783+49.5160,2461093.6803,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.7783+49.5160 20260222.1803 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:05.41 +49:30:51.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.80 01:41:50.30 +48:40:04.3
131.44763 -13.36877 galactic And Second-epoch detections are separated by 2.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405352278887767040 | 01:41:49.75 +48:40:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 50.30 +48 40 04.3 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405352278887767040,2461093.6803,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405352278887767040 20260222.1803 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:50.30 +48:40:04.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.66 01:42:51.28 +47:36:14.0
131.84004 -14.37656 galactic And Second-epoch detections are separated by 6.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351263522347996032 | 01:42:50.38 +47:36:16.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 51.28 +47 36 14.0 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351263522347996032,2461093.6803,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351263522347996032 20260222.1803 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:51.28 +47:36:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.74 01:39:39.94 +47:00:40.7
131.41383 -15.06464 galactic And Second-epoch detections are separated by 6.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399144474894943104 | 01:39:39.33 +47:00:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 39.94 +47 00 40.7 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399144474894943104,2461093.6803,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399144474894943104 20260222.1803 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:39.94 +47:00:40.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.58 01:38:44.23 +48:52:47.3
130.89036 -13.25968 galactic And Second-epoch detections are separated by 8.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.6924+48.8745 | 01:38:43.36 +48:52:50.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 44.23 +48 52 47.3 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.6924+48.8745,2461093.6803,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.6924+48.8745 20260222.1803 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:44.23 +48:52:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.65 01:43:28.37 +42:52:41.6
132.97759 -18.97625 galactic And Second-epoch detections are separated by 5.5" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347865619101026560 | 01:43:28.15 +42:52:34.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 28.37 +42 52 41.6 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347865619101026560,2461093.6803,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347865619101026560 20260222.1803 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:28.37 +42:52:41.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.72 01:49:50.70 +49:46:20.0
132.51375 -12.00978 galactic Per Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357860729553376256 | 01:49:51.28 +49:46:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 49 50.70 +49 46 20.0 13.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357860729553376256,2461093.6803,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357860729553376256 20260222.1803 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:49:50.70 +49:46:20.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.69 01:44:20.56 +44:14:23.3
132.83468 -17.61231 galactic And Second-epoch detections are separated by 3.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350211603254206976 | 01:44:21.38 +44:14:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 20.56 +44 14 23.3 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350211603254206976,2461093.6803,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350211603254206976 20260222.1803 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:20.56 +44:14:23.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.63 01:43:03.01 +45:47:14.3
132.26127 -16.14743 galactic And Second-epoch detections are separated by 3.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350624744748508672 | 01:43:03.78 +45:47:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 03.01 +45 47 14.3 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350624744748508672,2461093.6803,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350624744748508672 20260222.1803 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:03.01 +45:47:14.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.71 01:47:08.59 +48:09:21.2
132.44343 -13.68442 galactic And Second-epoch detections are separated by 6.8" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357248061058017024 | 01:47:09.28 +48:09:22.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 08.59 +48 09 21.2 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357248061058017024,2461093.6803,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357248061058017024 20260222.1803 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:08.59 +48:09:21.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.59 01:59:16.34 +50:55:48.0
133.70842 -10.51689 galactic Per Second-epoch detections are separated by 3.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J029.8216+50.9375 | 01:59:16.34 +50:55:48.0 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 59 16.34 +50 55 48.0 13.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J029.8216+50.9375,2461093.6803,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J029.8216+50.9375 20260222.1803 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:59:16.34 +50:55:48.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.59 01:46:56.64 +43:04:52.0
133.58521 -18.63951 galactic And Second-epoch detections are separated by 5.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 349335807882794624 | 01:46:57.34 +43:04:53.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 56.64 +43 04 52.0 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 349335807882794624,2461093.6803,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 349335807882794624 20260222.1803 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:56.64 +43:04:52.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.49 01:50:45.68 +49:47:12.6
132.65743 -11.96138 galactic Per Second-epoch detections are separated by 5.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357814897960006912 | 01:50:45.04 +49:47:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 50 45.68 +49 47 12.6 13.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357814897960006912,2461093.6803,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357814897960006912 20260222.1803 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:50:45.68 +49:47:12.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.65 01:44:23.44 +47:33:26.0
132.11162 -14.36849 galactic And Second-epoch detections are separated by 1.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351248644579527552 | 01:44:24.28 +47:33:29.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.733+/-0.127 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 23.44 +47 33 26.0 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351248644579527552,2461093.6803,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351248644579527552 20260222.1803 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:23.44 +47:33:26.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.55 01:44:24.54 +43:41:13.4
132.97128 -18.14969 galactic And Second-epoch detections are separated by 3.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350159234714845440 | 01:44:25.27 +43:41:18.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 24.54 +43 41 13.4 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350159234714845440,2461093.6803,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350159234714845440 20260222.1803 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:24.54 +43:41:13.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.66 01:45:29.89 +43:20:45.9
133.25219 -18.43971 galactic And Second-epoch detections are separated by 1.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 349399476477728384 | 01:45:29.80 +43:20:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 29.89 +43 20 45.9 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 349399476477728384,2461093.6803,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 349399476477728384 20260222.1803 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:29.89 +43:20:45.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.56 01:47:43.77 +41:03:06.3
134.22750 -20.58207 galactic And Second-epoch detections are separated by 8.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347396711750994944 | 01:47:44.54 +41:03:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 43.77 +41 03 06.3 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347396711750994944,2461093.6803,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347396711750994944 20260222.1803 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:43.77 +41:03:06.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.63 01:44:28.02 +45:05:11.2
132.66816 -16.78046 galactic And Second-epoch detections are separated by 3.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350379137040455808 | 01:44:28.98 +45:05:14.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 28.02 +45 05 11.2 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350379137040455808,2461093.6803,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350379137040455808 20260222.1803 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:28.02 +45:05:11.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.41 01:43:42.62 +43:18:01.9
132.92776 -18.55435 galactic And Second-epoch detections are separated by 8.3" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348652147870582912 | 01:43:43.07 +43:18:08.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 42.62 +43 18 01.9 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348652147870582912,2461093.6803,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348652147870582912 20260222.1803 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:42.62 +43:18:01.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 50.50 +46 01 37.8 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350645463670692608,2461093.6803,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350645463670692608 20260222.1803 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:50.50 +46:01:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.61 01:44:45.60 +43:15:53.0
133.13268 -18.54838 galactic And Second-epoch detections are separated by 2.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347901082646873728 | 01:44:46.27 +43:15:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5) J-Ks=0.746+/-0.221 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 45.60 +43 15 53.0 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347901082646873728,2461093.6803,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347901082646873728 20260222.1803 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:45.60 +43:15:53.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.52 01:51:11.71 +41:34:55.6
134.76693 -19.91228 galactic And Second-epoch detections are separated by 0.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347519410376478336 | 01:51:12.24 +41:35:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 51 11.71 +41 34 55.6 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347519410376478336,2461093.6803,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347519410376478336 20260222.1803 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:11.71 +41:34:55.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.41 01:44:48.52 +43:53:13.2
133.00011 -17.93890 galactic And Second-epoch detections are separated by 2.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350168000746287616 | 01:44:49.61 +43:53:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 48.52 +43 53 13.2 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350168000746287616,2461093.6803,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350168000746287616 20260222.1803 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:48.52 +43:53:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.43 01:43:16.49 +45:50:28.8
132.28947 -16.08646 galactic And Second-epoch detections are separated by 6.4" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.8294+45.8349 | 01:43:15.99 +45:50:32.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 16.49 +45 50 28.8 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.8294+45.8349,2461093.6803,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.8294+45.8349 20260222.1803 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:16.49 +45:50:28.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.39 01:41:20.14 +44:02:27.9
132.32393 -17.91882 galactic And Second-epoch detections are separated by 4.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350242935037912192 | 01:41:19.73 +44:02:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 20.14 +44 02 27.9 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350242935037912192,2461093.6803,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350242935037912192 20260222.1803 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:20.14 +44:02:27.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.35 01:45:48.81 +44:58:04.7
132.93755 -16.84478 galactic And Second-epoch detections are separated by 4.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350350481018587776 | 01:45:49.35 +44:58:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 48.81 +44 58 04.7 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350350481018587776,2461093.6803,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350350481018587776 20260222.1803 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:48.81 +44:58:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.30 01:40:15.25 +46:10:41.1
131.68449 -15.86240 galactic And Second-epoch detections are separated by 4.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350697136419667968 | 01:40:15.68 +46:10:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 15.25 +46 10 41.1 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350697136419667968,2461093.6803,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350697136419667968 20260222.1803 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:15.25 +46:10:41.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.20 01:51:13.32 +50:27:20.2
132.57132 -11.29384 galactic Per Second-epoch detections are separated by 6.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357976728028658560 | 01:51:12.43 +50:27:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 51 13.32 +50 27 20.2 13.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357976728028658560,2461093.6803,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357976728028658560 20260222.1803 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:13.32 +50:27:20.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.24 01:42:16.45 +46:55:29.1
131.88330 -15.06153 galactic And Second-epoch detections are separated by 1.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351118283733551616 | 01:42:17.30 +46:55:28.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 16.45 +46 55 29.1 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351118283733551616,2461093.6803,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351118283733551616 20260222.1803 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:16.45 +46:55:29.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.25 01:42:40.68 +42:38:43.6
132.87849 -19.23451 galactic And Second-epoch detections are separated by 5.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348607037832007936 | 01:42:41.26 +42:38:50.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 40.68 +42 38 43.6 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348607037832007936,2461093.6803,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348607037832007936 20260222.1803 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:40.68 +42:38:43.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.27 01:46:08.35 +42:12:53.9
133.63812 -19.51678 galactic And Second-epoch detections are separated by 1.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.5375+42.2197 | 01:46:08.88 +42:12:56.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 08.35 +42 12 53.9 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.5375+42.2197,2461093.6803,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.5375+42.2197 20260222.1803 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:08.35 +42:12:53.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.06 01:51:14.68 +50:50:07.4
132.48433 -10.92376 galactic Per Second-epoch detections are separated by 3.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J027.8074+50.8335 | 01:51:14.03 +50:50:10.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 51 14.68 +50 50 07.4 13.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J027.8074+50.8335,2461093.6803,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J027.8074+50.8335 20260222.1803 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:14.68 +50:50:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.02 01:41:39.06 +48:45:55.3
131.39656 -13.27937 galactic And Second-epoch detections are separated by 7.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405357230987706240 | 01:41:38.47 +48:45:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 39.06 +48 45 55.3 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405357230987706240,2461093.6803,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405357230987706240 20260222.1803 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:39.06 +48:45:55.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.98 01:46:14.29 +42:48:52.8
133.51530 -18.92812 galactic And Second-epoch detections are separated by 1.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347829786189987584 | 01:46:13.73 +42:48:50.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 14.29 +42 48 52.8 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347829786189987584,2461093.6803,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347829786189987584 20260222.1803 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:14.29 +42:48:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.02 01:44:22.30 +46:13:23.0
132.39979 -15.67331 galactic And Second-epoch detections are separated by 2.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351034828225647104 | 01:44:23.03 +46:13:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 22.30 +46 13 23.0 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351034828225647104,2461093.6803,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351034828225647104 20260222.1803 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:22.30 +46:13:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.93 01:39:48.75 +47:33:06.6
131.33144 -14.52943 galactic And Second-epoch detections are separated by 5.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399196044564387968 | 01:39:47.82 +47:33:06.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 48.75 +47 33 06.6 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399196044564387968,2461093.6803,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399196044564387968 20260222.1803 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:48.75 +47:33:06.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.85 01:44:10.11 +45:00:10.4
132.63289 -16.87331 galactic And Second-epoch detections are separated by 6.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350379897252559872 | 01:44:10.83 +45:00:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 10.11 +45 00 10.4 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350379897252559872,2461093.6803,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350379897252559872 20260222.1803 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:10.11 +45:00:10.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.96 01:48:18.99 +49:06:03.5
132.42181 -12.71989 galactic Per Second-epoch detections are separated by 2.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357440892206503296 | 01:48:19.61 +49:06:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 18.99 +49 06 03.5 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357440892206503296,2461093.6803,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357440892206503296 20260222.1803 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:18.99 +49:06:03.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.81 01:48:16.75 +42:23:33.7
134.00376 -19.25376 galactic And Second-epoch detections are separated by 0.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347618576877994624 | 01:48:16.13 +42:23:29.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 16.75 +42 23 33.7 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347618576877994624,2461093.6803,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347618576877994624 20260222.1803 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:16.75 +42:23:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.68 01:51:15.90 +49:44:40.3
132.74837 -11.98349 galactic Per Second-epoch detections are separated by 5.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357811530704590720 | 01:51:15.29 +49:44:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 51 15.90 +49 44 40.3 12.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357811530704590720,2461093.6803,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357811530704590720 20260222.1803 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:15.90 +49:44:40.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.80 01:42:12.31 +48:06:19.6
131.62506 -13.90755 galactic And Second-epoch detections are separated by 7.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399318129012680576 | 01:42:11.53 +48:06:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 12.31 +48 06 19.6 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399318129012680576,2461093.6803,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399318129012680576 20260222.1803 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:12.31 +48:06:19.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.81 01:44:07.77 +43:59:54.7
132.84948 -17.85619 galactic And Second-epoch detections are separated by 1.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350184115463564928 | 01:44:08.55 +43:59:54.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 07.77 +43 59 54.7 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350184115463564928,2461093.6803,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350184115463564928 20260222.1803 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:07.77 +43:59:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.73 02:15:26.80 +47:49:30.1
137.21244 -12.70377 galactic And Second-epoch detections are separated by 8.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 354791034823313664 | 02:15:29.42 +47:49:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 15 26.80 +47 49 30.1 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 354791034823313664,2461093.6803,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 354791034823313664 20260222.1803 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:15:26.80 +47:49:30.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.55 01:39:42.90 +46:08:02.0
131.59820 -15.92392 galactic And Second-epoch detections are separated by 7.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350702844433501568 | 01:39:42.40 +46:07:55.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 42.90 +46 08 02.0 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350702844433501568,2461093.6803,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350702844433501568 20260222.1803 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:42.90 +46:08:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.46 01:53:18.35 +50:20:13.6
132.92903 -11.32987 galactic Per Second-epoch detections are separated by 2.2" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357948763499843200 | 01:53:22.16 +50:20:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 53 18.35 +50 20 13.6 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357948763499843200,2461093.6803,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357948763499843200 20260222.1803 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:18.35 +50:20:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.34 01:46:55.49 +43:52:12.9
133.39490 -17.87133 galactic And Second-epoch detections are separated by 5.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 349442941546797696 | 01:46:55.93 +43:52:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 55.49 +43 52 12.9 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 349442941546797696,2461093.6803,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 349442941546797696 20260222.1803 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:55.49 +43:52:12.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.29 01:44:08.34 +44:31:52.3
132.73232 -17.33537 galactic And Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350224969192395008 | 01:44:09.12 +44:31:55.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 08.34 +44 31 52.3 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350224969192395008,2461093.6803,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350224969192395008 20260222.1803 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:08.34 +44:31:52.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.09 01:46:51.96 +48:49:14.8
132.24729 -13.04585 galactic And Second-epoch detections are separated by 0.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357410140240527744 | 01:46:51.37 +48:49:16.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 51.96 +48 49 14.8 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357410140240527744,2461093.6803,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357410140240527744 20260222.1803 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:51.96 +48:49:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.14 01:47:43.06 +41:11:40.9
134.18993 -20.44350 galactic And Second-epoch detections are separated by 8.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347407298847544832 | 01:47:43.53 +41:11:48.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 43.06 +41 11 40.9 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347407298847544832,2461093.6803,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347407298847544832 20260222.1803 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:43.06 +41:11:40.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.49 01:45:06.35 +45:11:59.2
132.75767 -16.64561 galactic And Second-epoch detections are separated by 8.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.2658+45.1951 | 01:45:06.91 +45:12:01.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 06.35 +45 11 59.2 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.2658+45.1951,2461093.6803,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.2658+45.1951 20260222.1803 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:06.35 +45:11:59.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.52 01:44:58.59 +44:13:14.9
132.95530 -17.60647 galactic And Second-epoch detections are separated by 6.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350204589569873408 | 01:44:59.33 +44:13:18.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 58.59 +44 13 14.9 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350204589569873408,2461093.6803,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350204589569873408 20260222.1803 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:58.59 +44:13:14.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.54 01:41:56.40 +42:51:51.8
132.69014 -19.04842 galactic And Second-epoch detections are separated by 2.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348613153865417088 | 01:41:57.01 +42:51:56.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 56.40 +42 51 51.8 10.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348613153865417088,2461093.6803,10.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348613153865417088 20260222.1803 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:56.40 +42:51:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.72 01:42:02.82 +48:01:53.7
131.61370 -13.98522 galactic And Second-epoch detections are separated by 4.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.5224+48.0287 | 01:42:03.33 +48:01:57.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 02.82 +48 01 53.7 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.5224+48.0287,2461093.6803,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.5224+48.0287 20260222.1803 10.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:02.82 +48:01:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.74 01:40:49.45 +47:23:59.4
131.53528 -14.64525 galactic And Second-epoch detections are separated by 2.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.2037+47.3897 | 01:40:50.30 +47:24:01.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 49.45 +47 23 59.4 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.2037+47.3897,2461093.6803,10.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.2037+47.3897 20260222.1803 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:49.45 +47:23:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.77 01:42:41.43 +50:53:46.8
131.12864 -11.15792 galactic Per Second-epoch detections are separated by 1.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406203854941373312 | 01:42:42.15 +50:53:44.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1927AnHar.100...33C HD 232509
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 41.43 +50 53 46.8 10.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406203854941373312,2461093.6803,10.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406203854941373312 20260222.1803 10.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:41.43 +50:53:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 10.87 01:43:13.44 +50:03:35.0
131.38640 -11.96001 galactic And Second-epoch detections are separated by 2.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405583691726395520 | 01:43:14.15 +50:03:32.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1952CoRut..32....1H BD+49 443
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 13.44 +50 03 35.0 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405583691726395520,2461093.6803,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405583691726395520 20260222.1803 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:13.44 +50:03:35.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.39 01:41:08.64 +47:06:56.6
131.64831 -14.91305 galactic And Second-epoch detections are separated by 5.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.2903+47.1042 | 01:41:09.50 +47:06:57.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 08.64 +47 06 56.6 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.2903+47.1042,2461093.6803,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.2903+47.1042 20260222.1803 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:08.64 +47:06:56.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.49 01:40:00.80 +48:48:14.8
131.11694 -13.29413 galactic And Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.9958+48.8013 | 01:40:01.41 +48:48:16.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 00.80 +48 48 14.8 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.9958+48.8013,2461093.6803,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.9958+48.8013 20260222.1803 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:00.80 +48:48:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.49 01:39:44.19 +49:12:13.0
130.99257 -12.91074 galactic And Second-epoch detections are separated by 4.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405425087173383680 | 01:39:44.90 +49:12:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 44.19 +49 12 13.0 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405425087173383680,2461093.6803,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405425087173383680 20260222.1803 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:44.19 +49:12:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.45 01:42:42.91 +46:13:32.6
132.10813 -15.73041 galactic And Second-epoch detections are separated by 6.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.6752+46.2160 | 01:42:43.55 +46:13:34.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 42.91 +46 13 32.6 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.6752+46.2160,2461093.6803,11.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.6752+46.2160 20260222.1803 11.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:42.91 +46:13:32.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.57 01:44:04.60 +41:59:53.0
133.29229 -19.81230 galactic And Second-epoch detections are separated by 1.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347730589625595264 | 01:44:05.16 +41:59:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 04.60 +41 59 53.0 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347730589625595264,2461093.6803,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347730589625595264 20260222.1803 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:04.60 +41:59:53.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.68 01:41:33.08 +47:09:26.5
131.70998 -14.85846 galactic And Second-epoch detections are separated by 5.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351134849423650304 | 01:41:33.96 +47:09:27.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 33.08 +47 09 26.5 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351134849423650304,2461093.6803,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351134849423650304 20260222.1803 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:33.08 +47:09:26.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.64 01:42:53.94 +42:39:53.6
132.91625 -19.20699 galactic And Second-epoch detections are separated by 0.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348606930454857856 | 01:42:54.86 +42:39:59.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 53.94 +42 39 53.6 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348606930454857856,2461093.6803,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348606930454857856 20260222.1803 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:53.94 +42:39:53.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.54 01:41:24.25 +43:03:13.1
132.54772 -18.88324 galactic And Second-epoch detections are separated by 6.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348631261447486464 | 01:41:24.80 +43:03:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 24.25 +43 03 13.1 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348631261447486464,2461093.6803,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348631261447486464 20260222.1803 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:24.25 +43:03:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.71 01:45:14.26 +50:43:02.9
131.56764 -11.24999 galactic Per Second-epoch detections are separated by 3.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.3228+50.7229 | 01:45:14.92 +50:43:01.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 14.26 +50 43 02.9 11.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.3228+50.7229,2461093.6803,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.3228+50.7229 20260222.1803 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:14.26 +50:43:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.76 01:42:19.97 +46:30:39.4
131.98061 -15.46467 galactic And Second-epoch detections are separated by 1.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351033900512508416 | 01:42:21.12 +46:30:42.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 19.97 +46 30 39.4 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351033900512508416,2461093.6803,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351033900512508416 20260222.1803 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:19.97 +46:30:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.71 01:42:25.71 +43:04:53.1
132.73516 -18.81762 galactic And Second-epoch detections are separated by 1.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348622087397329664 | 01:42:26.60 +43:04:59.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 25.71 +43 04 53.1 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348622087397329664,2461093.6803,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348622087397329664 20260222.1803 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:25.71 +43:04:53.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.79 01:43:03.08 +49:14:44.3
131.52823 -12.76270 galactic And Second-epoch detections are separated by 2.1" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405483876685721600 | 01:43:04.02 +49:14:43.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 03.08 +49 14 44.3 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405483876685721600,2461093.6803,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405483876685721600 20260222.1803 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:03.08 +49:14:44.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.78 01:40:54.32 +45:53:13.6
131.85938 -16.12541 galactic And Second-epoch detections are separated by 1.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350637904528061696 | 01:40:55.05 +45:53:16.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 54.32 +45 53 13.6 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350637904528061696,2461093.6803,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350637904528061696 20260222.1803 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:54.32 +45:53:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.80 01:44:36.89 +50:20:54.7
131.54797 -11.63149 galactic And Second-epoch detections are separated by 0.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405966497868961024 | 01:44:38.00 +50:20:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 36.89 +50 20 54.7 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405966497868961024,2461093.6803,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405966497868961024 20260222.1803 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:36.89 +50:20:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.80 01:48:20.88 +50:22:19.2
132.13615 -11.47992 galactic Per Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405931588375277952 | 01:48:21.70 +50:22:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 20.88 +50 22 19.2 11.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405931588375277952,2461093.6803,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405931588375277952 20260222.1803 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:20.88 +50:22:19.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.76 01:42:34.81 +46:57:03.4
131.93074 -15.02526 galactic And Second-epoch detections are separated by 4.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351115741111549952 | 01:42:35.65 +46:57:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 34.81 +46 57 03.4 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351115741111549952,2461093.6803,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351115741111549952 20260222.1803 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:34.81 +46:57:03.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.86 01:44:23.22 +50:23:38.7
131.50200 -11.59451 galactic And Second-epoch detections are separated by 2.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.0899+50.3935 | 01:44:24.11 +50:23:38.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: OB 1965ZA.....62....6B G 173- 16
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 23.22 +50 23 38.7 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.0899+50.3935,2461093.6803,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.0899+50.3935 20260222.1803 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:23.22 +50:23:38.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.85 01:40:18.39 +49:31:07.5
131.02392 -12.58364 galactic And Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.0953+49.5115 | 01:40:19.25 +49:31:08.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 18.39 +49 31 07.5 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.0953+49.5115,2461093.6803,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.0953+49.5115 20260222.1803 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:18.39 +49:31:07.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.87 01:43:53.92 +42:44:53.9
133.08755 -19.08657 galactic And Second-epoch detections are separated by 2.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.9841+42.7582 | 01:43:54.57 +42:44:58.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 53.92 +42 44 53.9 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.9841+42.7582,2461093.6803,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.9841+42.7582 20260222.1803 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:53.92 +42:44:53.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 48.43 +46 32 32.1 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351081832348032640,2461093.6803,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351081832348032640 20260222.1803 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:48.43 +46:32:32.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.75 01:48:14.51 +41:15:36.5
134.27602 -20.35699 galactic And Second-epoch detections are separated by 6.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347408604518236800 | 01:48:14.86 +41:15:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 14.51 +41 15 36.5 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347408604518236800,2461093.6803,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347408604518236800 20260222.1803 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:14.51 +41:15:36.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.92 01:40:50.14 +44:36:25.6
132.11275 -17.38227 galactic And Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350448273132186496 | 01:40:50.70 +44:36:27.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 50.14 +44 36 25.6 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350448273132186496,2461093.6803,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350448273132186496 20260222.1803 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:50.14 +44:36:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.97 01:45:17.34 +49:27:14.3
131.84911 -12.48313 galactic And Second-epoch detections are separated by 1.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405501885486463488 | 01:45:18.25 +49:27:14.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 17.34 +49 27 14.3 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405501885486463488,2461093.6803,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405501885486463488 20260222.1803 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:17.34 +49:27:14.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.01 01:46:38.45 +50:55:54.7
131.74158 -10.99321 galactic Per Second-epoch detections are separated by 5.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406051740082594432 | 01:46:39.24 +50:55:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 38.45 +50 55 54.7 12.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406051740082594432,2461093.6803,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406051740082594432 20260222.1803 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:38.45 +50:55:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.09 01:51:10.81 +50:11:41.3
132.62699 -11.54896 galactic Per Second-epoch detections are separated by 6.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357966596203869696 | 01:51:11.73 +50:11:41.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 51 10.81 +50 11 41.3 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357966596203869696,2461093.6803,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357966596203869696 20260222.1803 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:10.81 +50:11:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.02 01:46:26.56 +41:33:31.6
133.85309 -20.14358 galactic And Second-epoch detections are separated by 2.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347476774235574912 | 01:46:27.00 +41:33:36.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 26.56 +41 33 31.6 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347476774235574912,2461093.6803,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347476774235574912 20260222.1803 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:26.56 +41:33:31.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.06 01:47:21.67 +40:56:47.3
134.18117 -20.70053 galactic And Second-epoch detections are separated by 2.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347394482665196928 | 01:47:22.34 +40:56:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 21.67 +40 56 47.3 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347394482665196928,2461093.6803,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347394482665196928 20260222.1803 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:21.67 +40:56:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.14 01:44:46.48 +50:03:43.0
131.63480 -11.90637 galactic And Second-epoch detections are separated by 4.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405909323264398848 | 01:44:47.49 +50:03:40.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 46.48 +50 03 43.0 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405909323264398848,2461093.6803,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405909323264398848 20260222.1803 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:46.48 +50:03:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.12 01:42:40.02 +48:22:31.7
131.64638 -13.62755 galactic And Second-epoch detections are separated by 3.7" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405327780394319232 | 01:42:40.87 +48:22:33.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 40.02 +48 22 31.7 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405327780394319232,2461093.6803,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405327780394319232 20260222.1803 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:40.02 +48:22:31.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.12 01:41:58.33 +45:40:22.7
132.09389 -16.29788 galactic And Second-epoch detections are separated by 0.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350618834873543040 | 01:41:59.06 +45:40:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 58.33 +45 40 22.7 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350618834873543040,2461093.6803,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350618834873543040 20260222.1803 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:58.33 +45:40:22.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.07 01:42:24.03 +47:31:31.3
131.77910 -14.46904 galactic And Second-epoch detections are separated by 2.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351238890711237760 | 01:42:24.69 +47:31:34.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 24.03 +47 31 31.3 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351238890711237760,2461093.6803,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351238890711237760 20260222.1803 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:24.03 +47:31:31.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.07 01:42:11.68 +49:58:09.9
131.23945 -12.08184 galactic And Second-epoch detections are separated by 5.7" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405588472026941184 | 01:42:12.46 +49:58:12.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 11.68 +49 58 09.9 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405588472026941184,2461093.6803,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405588472026941184 20260222.1803 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:11.68 +49:58:09.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.20 01:44:13.52 +50:47:28.3
131.39230 -11.21138 galactic Per Second-epoch detections are separated by 3.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 406012333759725952 | 01:44:14.60 +50:47:26.5 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 13.52 +50 47 28.3 12.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 406012333759725952,2461093.6803,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 406012333759725952 20260222.1803 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:13.52 +50:47:28.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.16 01:44:21.12 +42:00:18.3
133.34376 -19.79440 galactic And Second-epoch detections are separated by 5.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347730108589709440 | 01:44:21.59 +42:00:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 21.12 +42 00 18.3 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347730108589709440,2461093.6803,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347730108589709440 20260222.1803 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:21.12 +42:00:18.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.17 01:42:55.33 +49:06:37.4
131.53528 -12.89942 galactic And Second-epoch detections are separated by 2.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405388945026313600 | 01:42:56.21 +49:06:39.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 55.33 +49 06 37.4 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405388945026313600,2461093.6803,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405388945026313600 20260222.1803 12.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:55.33 +49:06:37.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.26 01:47:26.71 +49:57:44.8
132.08488 -11.91133 galactic And Second-epoch detections are separated by 2.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357857916351050752 | 01:47:27.67 +49:57:46.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 26.71 +49 57 44.8 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357857916351050752,2461093.6803,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357857916351050752 20260222.1803 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:26.71 +49:57:44.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.13 01:39:35.57 +49:52:19.9
130.83864 -12.25884 galactic And Second-epoch detections are separated by 0.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405748313529963136 | 01:39:36.54 +49:52:20.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 35.57 +49 52 19.9 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405748313529963136,2461093.6803,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405748313529963136 20260222.1803 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:35.57 +49:52:19.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.05 01:44:35.93 +47:22:04.6
132.18835 -14.54610 galactic And Second-epoch detections are separated by 6.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351198861616090880 | 01:44:36.64 +47:22:05.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 35.93 +47 22 04.6 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351198861616090880,2461093.6803,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351198861616090880 20260222.1803 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:35.93 +47:22:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.23 01:44:46.84 +49:40:24.1
131.71919 -12.28609 galactic And Second-epoch detections are separated by 2.7" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405520302306131840 | 01:44:47.95 +49:40:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 46.84 +49 40 24.1 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405520302306131840,2461093.6803,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405520302306131840 20260222.1803 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:46.84 +49:40:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.23 01:44:36.47 +41:24:56.4
133.52978 -20.35935 galactic And Second-epoch detections are separated by 1.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347635550589371136 | 01:44:37.06 +41:25:02.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 36.47 +41 24 56.4 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347635550589371136,2461093.6803,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347635550589371136 20260222.1803 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:36.47 +41:24:56.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.25 01:46:55.09 +41:29:32.4
133.96146 -20.18816 galactic And Second-epoch detections are separated by 2.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347472513630898944 | 01:46:55.61 +41:29:38.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5) J-Ks=0.819+/-0.043 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 55.09 +41 29 32.4 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347472513630898944,2461093.6803,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347472513630898944 20260222.1803 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:55.09 +41:29:32.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.29 01:44:38.66 +40:54:01.1
133.65736 -20.86073 galactic And Second-epoch detections are separated by 1.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347429323439733632 | 01:44:39.18 +40:54:05.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 38.66 +40 54 01.1 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347429323439733632,2461093.6803,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347429323439733632 20260222.1803 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:38.66 +40:54:01.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.36 01:46:54.82 +50:17:09.6
131.92761 -11.61428 galactic And Second-epoch detections are separated by 3.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405927392189164160 | 01:46:55.92 +50:17:05.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 54.82 +50 17 09.6 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405927392189164160,2461093.6803,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405927392189164160 20260222.1803 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:54.82 +50:17:09.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.36 01:47:08.56 +49:42:19.1
132.09395 -12.17291 galactic And Second-epoch detections are separated by 4.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357847952026978688 | 01:47:09.34 +49:42:16.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 08.56 +49 42 19.1 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357847952026978688,2461093.6803,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357847952026978688 20260222.1803 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:08.56 +49:42:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.30 01:45:39.66 +50:02:45.0
131.78039 -11.89203 galactic And Second-epoch detections are separated by 5.8" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405906913784507264 | 01:45:40.60 +50:02:43.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 39.66 +50 02 45.0 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405906913784507264,2461093.6803,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405906913784507264 20260222.1803 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:39.66 +50:02:45.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.32 01:41:51.60 +46:18:24.2
131.94070 -15.68117 galactic And Second-epoch detections are separated by 4.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351025104419559296 | 01:41:52.48 +46:18:26.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 51.60 +46 18 24.2 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351025104419559296,2461093.6803,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351025104419559296 20260222.1803 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:51.60 +46:18:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.46 01:44:52.03 +41:57:29.3
133.45394 -19.81939 galactic And Second-epoch detections are separated by 5.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347687876173891456 | 01:44:53.27 +41:57:41.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 52.03 +41 57 29.3 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347687876173891456,2461093.6803,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347687876173891456 20260222.1803 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:52.03 +41:57:29.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.47 01:47:23.38 +40:55:35.7
134.19166 -20.71865 galactic And Second-epoch detections are separated by 3.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347394409647582208 | 01:47:23.98 +40:55:46.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 23.38 +40 55 35.7 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347394409647582208,2461093.6803,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347394409647582208 20260222.1803 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:23.38 +40:55:35.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.34 01:38:40.54 +48:48:07.7
130.89509 -13.33787 galactic And Second-epoch detections are separated by 2.7" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399411381342103040 | 01:38:41.37 +48:48:11.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 40.54 +48 48 07.7 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399411381342103040,2461093.6803,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399411381342103040 20260222.1803 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:40.54 +48:48:07.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.48 01:41:00.84 +48:47:27.9
131.28564 -13.27488 galactic And Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.2450+48.7990 | 01:41:01.27 +48:47:21.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 00.84 +48 47 27.9 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.2450+48.7990,2461093.6803,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.2450+48.7990 20260222.1803 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:00.84 +48:47:27.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.46 01:41:17.39 +46:27:17.1
131.80984 -15.55587 galactic And Second-epoch detections are separated by 1.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.3314+46.4448 | 01:41:18.28 +46:27:17.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 17.39 +46 27 17.1 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.3314+46.4448,2461093.6803,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.3314+46.4448 20260222.1803 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:17.39 +46:27:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.40 01:38:43.41 +47:54:49.2
131.07477 -14.20907 galactic And Second-epoch detections are separated by 1.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399345204486192768 | 01:38:44.01 +47:54:49.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 43.41 +47 54 49.2 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399345204486192768,2461093.6803,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399345204486192768 20260222.1803 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:43.41 +47:54:49.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.45 01:43:19.16 +41:23:19.1
133.28429 -20.43786 galactic And Second-epoch detections are separated by 2.6" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347641323025424384 | 01:43:19.59 +41:23:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 19.16 +41 23 19.1 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347641323025424384,2461093.6803,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347641323025424384 20260222.1803 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:19.16 +41:23:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.40 01:39:08.27 +49:01:15.3
130.92946 -13.10871 galactic And Second-epoch detections are separated by 2.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405419250315392896 | 01:39:09.15 +49:01:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 08.27 +49 01 15.3 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405419250315392896,2461093.6803,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405419250315392896 20260222.1803 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:08.27 +49:01:15.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.48 01:49:58.89 +50:47:44.2
132.29600 -11.00865 galactic Per Second-epoch detections are separated by 1.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357999822070616448 | 01:49:59.92 +50:47:41.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 49 58.89 +50 47 44.2 12.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357999822070616448,2461093.6803,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357999822070616448 20260222.1803 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:49:58.89 +50:47:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.47 01:44:56.88 +50:10:28.1
131.63840 -11.79052 galactic And Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.2413+50.1735 | 01:44:57.93 +50:10:24.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 56.88 +50 10 28.1 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.2413+50.1735,2461093.6803,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.2413+50.1735 20260222.1803 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:56.88 +50:10:28.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 28.81 +41 22 25.3 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347456501993432576,2461093.6803,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347456501993432576 20260222.1803 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:28.81 +41:22:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.51 01:46:54.10 +41:10:23.1
134.03571 -20.49974 galactic And Second-epoch detections are separated by 2.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347447740259611648 | 01:46:54.85 +41:10:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 54.10 +41 10 23.1 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347447740259611648,2461093.6803,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347447740259611648 20260222.1803 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:54.10 +41:10:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.43 01:43:10.13 +49:54:13.0
131.41005 -12.11465 galactic And Second-epoch detections are separated by 7.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405573972217373312 | 01:43:10.94 +49:54:12.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 10.13 +49 54 13.0 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405573972217373312,2461093.6803,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405573972217373312 20260222.1803 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:10.13 +49:54:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.51 01:40:10.55 +45:21:39.5
131.83722 -16.66637 galactic And Second-epoch detections are separated by 3.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350599559060201728 | 01:40:11.12 +45:21:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 10.55 +45 21 39.5 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350599559060201728,2461093.6803,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350599559060201728 20260222.1803 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:10.55 +45:21:39.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.58 01:48:09.36 +50:53:40.7
131.98726 -10.97718 galactic Per Second-epoch detections are separated by 6.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406042467250830080 | 01:48:10.19 +50:53:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 09.36 +50 53 40.7 12.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406042467250830080,2461093.6803,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406042467250830080 20260222.1803 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:09.36 +50:53:40.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.55 01:42:50.80 +41:16:19.4
133.21814 -20.57062 galactic And Second-epoch detections are separated by 2.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347268103249366272 | 01:42:51.27 +41:16:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 50.80 +41 16 19.4 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347268103249366272,2461093.6803,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347268103249366272 20260222.1803 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:50.80 +41:16:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.54 01:41:44.33 +48:56:42.4
131.37439 -13.10034 galactic And Second-epoch detections are separated by 4.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.4490+48.9427 | 01:41:44.95 +48:56:44.8 (Gaia DR3) | CBH (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 44.33 +48 56 42.4 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.4490+48.9427,2461093.6803,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.4490+48.9427 20260222.1803 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:44.33 +48:56:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.68 01:49:10.98 +50:08:40.1
132.32112 -11.67161 galactic Per Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357886950330113024 | 01:49:11.90 +50:08:38.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 49 10.98 +50 08 40.1 12.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357886950330113024,2461093.6803,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357886950330113024 20260222.1803 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:49:10.98 +50:08:40.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.62 01:41:13.72 +49:57:03.7
131.08743 -12.13063 galactic And Second-epoch detections are separated by 1.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405568268500606080 | 01:41:14.62 +49:57:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 13.72 +49 57 03.7 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405568268500606080,2461093.6803,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405568268500606080 20260222.1803 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:13.72 +49:57:03.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.66 01:41:37.25 +49:31:01.5
131.23859 -12.54357 galactic And Second-epoch detections are separated by 2.0" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.4247+49.5231 | 01:41:38.16 +49:30:59.7 (Gaia DR3) | DBF (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 37.25 +49 31 01.5 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.4247+49.5231,2461093.6803,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.4247+49.5231 20260222.1803 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:37.25 +49:31:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.70 01:48:07.32 +50:18:38.5
132.11421 -11.54772 galactic Per Second-epoch detections are separated by 1.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405930935540034688 | 01:48:08.06 +50:18:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 07.32 +50 18 38.5 12.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405930935540034688,2461093.6803,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405930935540034688 20260222.1803 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:07.32 +50:18:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.63 01:43:50.29 +48:14:20.1
131.87139 -13.72121 galactic And Second-epoch detections are separated by 3.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 357287029297613824 | 01:43:51.29 +48:14:20.0 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 50.29 +48 14 20.1 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 357287029297613824,2461093.6803,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 357287029297613824 20260222.1803 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:50.29 +48:14:20.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.65 01:42:46.68 +41:03:48.1
133.25180 -20.77733 galactic And Second-epoch detections are separated by 2.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347261132519796480 | 01:42:47.26 +41:03:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 46.68 +41 03 48.1 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347261132519796480,2461093.6803,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347261132519796480 20260222.1803 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:46.68 +41:03:48.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 03.62 +47 46 53.4 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399295966981346048,2461093.6803,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399295966981346048 20260222.1803 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:03.62 +47:46:53.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.77 01:42:37.78 +48:32:05.4
131.60689 -13.47276 galactic And Second-epoch detections are separated by 7.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405338053956086528 | 01:42:38.67 +48:32:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 37.78 +48 32 05.4 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405338053956086528,2461093.6803,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405338053956086528 20260222.1803 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:37.78 +48:32:05.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.67 01:40:24.35 +45:31:10.9
131.84596 -16.50281 galactic And Second-epoch detections are separated by 2.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350602956377518464 | 01:40:25.02 +45:31:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 24.35 +45 31 10.9 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350602956377518464,2461093.6803,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350602956377518464 20260222.1803 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:24.35 +45:31:10.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.74 01:40:28.67 +50:36:02.1
130.83810 -11.51683 galactic And Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405798233933494656 | 01:40:29.47 +50:35:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 28.67 +50 36 02.1 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405798233933494656,2461093.6803,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405798233933494656 20260222.1803 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:28.67 +50:36:02.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 31.26 +49 41 32.6 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405546037748025856,2461093.6803,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405546037748025856 20260222.1803 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:31.26 +49:41:32.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.72 01:42:22.98 +49:10:51.3
131.43206 -12.84819 galactic And Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405393235695936000 | 01:42:24.09 +49:10:51.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 22.98 +49 10 51.3 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405393235695936000,2461093.6803,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405393235695936000 20260222.1803 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:22.98 +49:10:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.68 01:47:37.68 +41:35:32.3
134.07482 -20.06047 galactic And Second-epoch detections are separated by 6.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347463167779152000 | 01:47:38.17 +41:35:37.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 37.68 +41 35 32.3 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347463167779152000,2461093.6803,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347463167779152000 20260222.1803 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:37.68 +41:35:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.71 01:42:18.20 +47:55:50.5
131.67796 -14.07540 galactic And Second-epoch detections are separated by 2.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399310329352092032 | 01:42:19.01 +47:55:53.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 18.20 +47 55 50.5 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399310329352092032,2461093.6803,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399310329352092032 20260222.1803 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:18.20 +47:55:50.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.62 01:42:15.65 +41:22:02.4
133.08192 -20.50060 galactic And Second-epoch detections are separated by 0.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347316245540071296 | 01:42:16.25 +41:22:12.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 15.65 +41 22 02.4 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347316245540071296,2461093.6803,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347316245540071296 20260222.1803 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:15.65 +41:22:02.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.78 01:44:47.49 +41:00:59.5
133.65909 -20.74124 galactic And Second-epoch detections are separated by 6.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347431728621410304 | 01:44:48.07 +41:01:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 47.49 +41 00 59.5 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347431728621410304,2461093.6803,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347431728621410304 20260222.1803 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:47.49 +41:00:59.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.74 01:44:37.14 +41:48:38.2
133.44023 -19.97345 galactic And Second-epoch detections are separated by 3.8" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347679531054409088 | 01:44:38.33 +41:48:48.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 37.14 +41 48 38.2 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347679531054409088,2461093.6803,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347679531054409088 20260222.1803 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:37.14 +41:48:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.73 01:47:07.75 +49:19:04.6
132.17871 -12.55132 galactic And Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357458793629893120 | 01:47:08.53 +49:19:03.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 07.75 +49 19 04.6 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357458793629893120,2461093.6803,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357458793629893120 20260222.1803 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:07.75 +49:19:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.68 01:46:38.82 +41:54:52.4
133.80724 -19.78837 galactic And Second-epoch detections are separated by 3.3" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347763609334084608 | 01:46:39.49 +41:55:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 38.82 +41 54 52.4 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347763609334084608,2461093.6803,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347763609334084608 20260222.1803 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:38.82 +41:54:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.72 01:42:10.20 +49:43:57.1
131.28393 -12.31474 galactic And Second-epoch detections are separated by 0.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405549301925298688 | 01:42:11.18 +49:43:55.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 10.20 +49 43 57.1 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405549301925298688,2461093.6803,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405549301925298688 20260222.1803 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:10.20 +49:43:57.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.79 01:41:46.28 +47:10:28.5
131.74432 -14.83410 galactic And Second-epoch detections are separated by 4.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351135085645609856 | 01:41:47.19 +47:10:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5) J-Ks=0.614+/-0.148 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 46.28 +47 10 28.5 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351135085645609856,2461093.6803,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351135085645609856 20260222.1803 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:46.28 +47:10:28.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 08.29 +50 46 10.9 12.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406010821931248384,2461093.6803,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406010821931248384 20260222.1803 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:08.29 +50:46:10.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.79 01:43:05.79 +49:47:23.6
131.42206 -12.22837 galactic And Second-epoch detections are separated by 1.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405571498316257920 | 01:43:06.46 +49:47:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 05.79 +49 47 23.6 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405571498316257920,2461093.6803,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405571498316257920 20260222.1803 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:05.79 +49:47:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.74 01:44:13.91 +49:20:00.7
131.70276 -12.63704 galactic And Second-epoch detections are separated by 2.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.0614+49.3336 | 01:44:14.74 +49:20:01.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 13.91 +49 20 00.7 12.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.0614+49.3336,2461093.6803,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.0614+49.3336 20260222.1803 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:13.91 +49:20:00.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.76 01:47:29.28 +41:23:13.3
134.09791 -20.26628 galactic And Second-epoch detections are separated by 1.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347456501993432576 | 01:47:29.35 +41:22:32.9 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 29.28 +41 23 13.3 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347456501993432576,2461093.6803,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347456501993432576 20260222.1803 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:29.28 +41:23:13.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.79 01:43:19.22 +44:53:54.6
132.50251 -17.00695 galactic And Second-epoch detections are separated by 2.0" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.8332+44.9060 | 01:43:20.30 +44:53:56.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 19.22 +44 53 54.6 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.8332+44.9060,2461093.6803,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.8332+44.9060 20260222.1803 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:19.22 +44:53:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.86 01:46:37.43 +49:51:27.9
131.97636 -12.04240 galactic And Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.6605+49.8604 | 01:46:38.36 +49:51:26.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.780+/-0.142 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 37.43 +49 51 27.9 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.6605+49.8604,2461093.6803,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.6605+49.8604 20260222.1803 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:37.43 +49:51:27.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.80 01:40:19.18 +48:29:58.1
131.22846 -13.58326 galactic And Second-epoch detections are separated by 4.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399389047512390912 | 01:40:19.05 +48:29:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 19.18 +48 29 58.1 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399389047512390912,2461093.6803,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399389047512390912 20260222.1803 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:19.18 +48:29:58.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.78 01:45:53.39 +42:19:49.6
133.56316 -19.41447 galactic And Second-epoch detections are separated by 0.5" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347790306850727424 | 01:45:53.88 +42:19:53.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 53.39 +42 19 49.6 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347790306850727424,2461093.6803,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347790306850727424 20260222.1803 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:53.39 +42:19:49.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.79 01:40:18.42 +50:12:24.0
130.88833 -11.90861 galactic And Second-epoch detections are separated by 3.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405785765644727680 | 01:40:19.13 +50:12:24.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 18.42 +50 12 24.0 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405785765644727680,2461093.6803,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405785765644727680 20260222.1803 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:18.42 +50:12:24.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.87 01:40:39.60 +50:29:38.0
130.88813 -11.61592 galactic And Second-epoch detections are separated by 4.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405795489450614656 | 01:40:40.76 +50:29:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 39.60 +50 29 38.0 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405795489450614656,2461093.6803,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405795489450614656 20260222.1803 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:39.60 +50:29:38.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.95 01:44:12.27 +50:35:01.8
131.43282 -11.41492 galactic And Second-epoch detections are separated by 1.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405974327591754240 | 01:44:13.28 +50:34:59.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 12.27 +50 35 01.8 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405974327591754240,2461093.6803,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405974327591754240 20260222.1803 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:12.27 +50:35:01.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.85 01:47:29.12 +49:53:59.1
132.10543 -11.97107 galactic And Second-epoch detections are separated by 6.3" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357857126077343360 | 01:47:29.94 +49:53:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 29.12 +49 53 59.1 12.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357857126077343360,2461093.6803,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357857126077343360 20260222.1803 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:29.12 +49:53:59.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.86 01:39:53.62 +46:26:13.6
131.56863 -15.62046 galactic And Second-epoch detections are separated by 4.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.9771+46.4262 | 01:39:54.48 +46:26:14.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 53.62 +46 26 13.6 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.9771+46.4262,2461093.6803,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.9771+46.4262 20260222.1803 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:53.62 +46:26:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.89 01:39:54.79 +48:44:41.4
131.11201 -13.35547 galactic And Second-epoch detections are separated by 6.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405399764046184576 | 01:39:54.99 +48:44:47.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 54.79 +48 44 41.4 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405399764046184576,2461093.6803,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405399764046184576 20260222.1803 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:54.79 +48:44:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.89 01:42:55.31 +50:35:01.2
131.22952 -11.45677 galactic And Second-epoch detections are separated by 3.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.7351+50.5830 | 01:42:56.44 +50:34:58.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 55.31 +50 35 01.2 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.7351+50.5830,2461093.6803,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.7351+50.5830 20260222.1803 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:55.31 +50:35:01.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 13.66 +47 34 34.4 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J013913.2+473456,2461093.6803,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J013913.2+473456 20260222.1803 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:13.66 +47:34:34.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.97 01:38:57.99 +48:26:44.1
131.01254 -13.67904 galactic And Second-epoch detections are separated by 2.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399385748977344256 | 01:38:58.58 +48:26:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 57.99 +48 26 44.1 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399385748977344256,2461093.6803,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399385748977344256 20260222.1803 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:57.99 +48:26:44.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.01 01:40:15.29 +47:01:23.3
131.51347 -15.03358 galactic And Second-epoch detections are separated by 2.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399167251104875136 | 01:40:16.14 +47:01:26.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 15.29 +47 01 23.3 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399167251104875136,2461093.6803,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399167251104875136 20260222.1803 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:15.29 +47:01:23.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.02 01:51:28.58 +50:40:50.0
132.55758 -11.06570 galactic Per Second-epoch detections are separated by 5.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 358006243043977984 | 01:51:29.32 +50:40:47.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 51 28.58 +50 40 50.0 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 358006243043977984,2461093.6803,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 358006243043977984 20260222.1803 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:28.58 +50:40:50.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.97 01:41:47.73 +50:48:42.9
131.00470 -11.26882 galactic Per Second-epoch detections are separated by 2.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406181722973717760 | 01:41:48.64 +50:48:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 47.73 +50 48 42.9 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406181722973717760,2461093.6803,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406181722973717760 20260222.1803 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:47.73 +50:48:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.95 01:41:28.15 +50:45:37.4
130.96350 -11.32950 galactic Per Second-epoch detections are separated by 0.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406175817394761216 | 01:41:29.02 +50:45:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 28.15 +50 45 37.4 12.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406175817394761216,2461093.6803,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406175817394761216 20260222.1803 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:28.15 +50:45:37.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.91 01:44:09.59 +48:57:04.9
131.77258 -13.01328 galactic And Second-epoch detections are separated by 4.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.0485+48.9638 | 01:44:10.46 +48:57:06.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 09.59 +48 57 04.9 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.0485+48.9638,2461093.6803,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.0485+48.9638 20260222.1803 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:09.59 +48:57:04.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 00.68 +50 24 37.4 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405975908139697408,2461093.6803,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405975908139697408 20260222.1803 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:00.68 +50:24:37.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 14.97 +45 31 37.8 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 3883583,2461093.6803,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3883583 20260222.1803 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:14.97 +45:31:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.06 01:42:57.72 +42:19:18.6
133.00472 -19.53994 galactic And Second-epoch detections are separated by 6.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347757935680929792 | 01:42:58.24 +42:19:21.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 57.72 +42 19 18.6 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347757935680929792,2461093.6803,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347757935680929792 20260222.1803 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:57.72 +42:19:18.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.97 01:42:50.32 +45:52:17.2
132.20566 -16.07271 galactic And Second-epoch detections are separated by 3.8" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.7202+45.8736 | 01:42:51.48 +45:52:18.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 50.32 +45 52 17.2 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.7202+45.8736,2461093.6803,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.7202+45.8736 20260222.1803 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:50.32 +45:52:17.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.11 01:43:37.77 +47:25:45.4
132.00939 -14.52048 galactic And Second-epoch detections are separated by 4.7" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351223527611613952 | 01:43:38.91 +47:25:47.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 37.77 +47 25 45.4 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351223527611613952,2461093.6803,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351223527611613952 20260222.1803 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:37.77 +47:25:45.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.05 01:41:30.75 +43:52:17.3
132.39281 -18.07847 galactic And Second-epoch detections are separated by 3.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348728087190363136 | 01:41:31.51 +43:52:21.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 30.75 +43 52 17.3 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348728087190363136,2461093.6803,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348728087190363136 20260222.1803 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:30.75 +43:52:17.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.12 01:47:08.66 +40:59:47.9
134.12629 -20.66109 galactic And Second-epoch detections are separated by 1.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347398537114311040 | 01:47:09.32 +40:59:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 08.66 +40 59 47.9 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347398537114311040,2461093.6803,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347398537114311040 20260222.1803 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:08.66 +40:59:47.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.96 01:42:29.49 +47:16:49.1
131.84608 -14.70587 galactic And Second-epoch detections are separated by 3.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351218579810416000 | 01:42:30.61 +47:16:49.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 29.49 +47 16 49.1 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351218579810416000,2461093.6803,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351218579810416000 20260222.1803 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:29.49 +47:16:49.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.99 01:42:15.76 +41:27:52.2
133.06061 -20.40550 galactic And Second-epoch detections are separated by 2.0" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.5612+41.4640 | 01:42:16.54 +41:27:52.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 15.76 +41 27 52.2 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.5612+41.4640,2461093.6803,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.5612+41.4640 20260222.1803 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:15.76 +41:27:52.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.08 01:42:51.08 +43:06:44.4
132.80810 -18.77130 galactic And Second-epoch detections are separated by 4.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348623049469991936 | 01:42:51.89 +43:06:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 51.08 +43 06 44.4 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348623049469991936,2461093.6803,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348623049469991936 20260222.1803 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:51.08 +43:06:44.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.10 01:43:36.69 +41:13:27.0
133.37907 -20.58679 galactic And Second-epoch detections are separated by 4.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347627338611935360 | 01:43:37.16 +41:13:31.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 36.69 +41 13 27.0 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347627338611935360,2461093.6803,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347627338611935360 20260222.1803 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:36.69 +41:13:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.07 01:44:10.00 +41:26:56.9
133.43594 -20.34465 galactic And Second-epoch detections are separated by 2.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347648121955863808 | 01:44:10.58 +41:27:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 10.00 +41 26 56.9 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347648121955863808,2461093.6803,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347648121955863808 20260222.1803 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:10.00 +41:26:56.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.10 01:42:55.50 +41:25:28.6
133.19903 -20.41841 galactic And Second-epoch detections are separated by 3.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347644930797776128 | 01:42:56.07 +41:25:35.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 55.50 +41 25 28.6 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347644930797776128,2461093.6803,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347644930797776128 20260222.1803 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:55.50 +41:25:28.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.15 01:46:27.43 +50:15:31.0
131.86098 -11.65684 galactic And Second-epoch detections are separated by 3.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405904439883936128 | 01:46:28.53 +50:15:28.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 27.43 +50 15 31.0 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405904439883936128,2461093.6803,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405904439883936128 20260222.1803 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:27.43 +50:15:31.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 12.96 01:46:43.96 +41:33:49.0
133.90821 -20.12662 galactic And Second-epoch detections are separated by 6.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347474055522073216 | 01:46:44.73 +41:33:54.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 43.96 +41 33 49.0 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347474055522073216,2461093.6803,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347474055522073216 20260222.1803 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:43.96 +41:33:49.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.12 01:40:58.36 +44:53:38.1
132.07778 -17.09637 galactic And Second-epoch detections are separated by 3.5" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350478853299311232 | 01:40:59.14 +44:53:37.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 58.36 +44 53 38.1 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350478853299311232,2461093.6803,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350478853299311232 20260222.1803 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:58.36 +44:53:38.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.05 01:43:42.36 +48:22:35.3
131.81992 -13.59120 galactic And Second-epoch detections are separated by 8.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.9203+48.3668 | 01:43:42.91 +48:22:41.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 42.36 +48 22 35.3 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.9203+48.3668,2461093.6803,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.9203+48.3668 20260222.1803 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:42.36 +48:22:35.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.15 01:40:07.54 +47:00:48.3
131.49307 -15.04740 galactic And Second-epoch detections are separated by 3.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399166911804187776 | 01:40:07.89 +47:00:59.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 07.54 +47 00 48.3 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399166911804187776,2461093.6803,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399166911804187776 20260222.1803 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:07.54 +47:00:48.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.10 01:37:53.81 +49:31:02.6
130.63057 -12.65863 galactic And Second-epoch detections are separated by 2.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405646466969431552 | 01:37:54.57 +49:31:01.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 37 53.81 +49 31 02.6 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405646466969431552,2461093.6803,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405646466969431552 20260222.1803 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:37:53.81 +49:31:02.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.01 01:41:03.82 +44:44:46.8
132.12521 -17.23775 galactic And Second-epoch detections are separated by 3.2" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350473355741186432 | 01:41:04.54 +44:44:46.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 03.82 +44 44 46.8 13.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350473355741186432,2461093.6803,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350473355741186432 20260222.1803 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:03.82 +44:44:46.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.17 01:39:23.28 +50:19:09.9
130.71904 -11.82593 galactic And Second-epoch detections are separated by 2.5" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 405775801318824064 | 01:39:24.09 +50:19:10.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 23.28 +50 19 09.9 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 405775801318824064,2461093.6803,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 405775801318824064 20260222.1803 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:23.28 +50:19:09.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.12 01:48:08.64 +49:34:01.7
132.28699 -12.27181 galactic Per Second-epoch detections are separated by 1.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357831528072448768 | 01:48:09.47 +49:34:01.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 08.64 +49 34 01.7 13.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357831528072448768,2461093.6803,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357831528072448768 20260222.1803 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:08.64 +49:34:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.12 01:44:47.42 +50:21:23.8
131.57419 -11.61773 galactic And Second-epoch detections are separated by 2.6" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405966704027388160 | 01:44:48.35 +50:21:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 47.42 +50 21 23.8 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405966704027388160,2461093.6803,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405966704027388160 20260222.1803 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:47.42 +50:21:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.12 01:45:59.06 +40:53:19.0
133.92434 -20.81596 galactic And Second-epoch detections are separated by 0.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347420458627422592 | 01:45:59.63 +40:53:25.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 59.06 +40 53 19.0 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347420458627422592,2461093.6803,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347420458627422592 20260222.1803 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:59.06 +40:53:19.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.13 01:40:05.34 +49:36:51.7
130.96961 -12.49661 galactic And Second-epoch detections are separated by 5.5" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405463844960429312 | 01:40:06.06 +49:36:52.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 05.34 +49 36 51.7 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405463844960429312,2461093.6803,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405463844960429312 20260222.1803 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:05.34 +49:36:51.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.24 01:44:22.23 +45:26:14.8
132.57290 -16.44111 galactic And Second-epoch detections are separated by 2.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350427691648531584 | 01:44:23.16 +45:26:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 22.23 +45 26 14.8 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350427691648531584,2461093.6803,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350427691648531584 20260222.1803 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:22.23 +45:26:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.22 01:41:37.79 +45:33:04.7
132.05843 -16.42914 galactic And Second-epoch detections are separated by 8.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350606224849593728 | 01:41:38.50 +45:33:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 37.79 +45 33 04.7 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350606224849593728,2461093.6803,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350606224849593728 20260222.1803 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:37.79 +45:33:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.09 01:43:29.86 +49:41:03.1
131.50909 -12.31859 galactic And Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405523046788198912 | 01:43:30.52 +49:41:01.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 29.86 +49 41 03.1 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405523046788198912,2461093.6803,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405523046788198912 20260222.1803 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:29.86 +49:41:03.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.21 01:44:31.98 +50:40:49.8
131.46430 -11.30954 galactic Per Second-epoch detections are separated by 5.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405997765230708352 | 01:44:32.86 +50:40:45.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 31.98 +50 40 49.8 13.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405997765230708352,2461093.6803,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405997765230708352 20260222.1803 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:31.98 +50:40:49.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.22 01:44:40.03 +41:26:50.8
133.53396 -20.32591 galactic And Second-epoch detections are separated by 5.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347637268576283904 | 01:44:40.81 +41:27:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.384+/-0.166 (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 40.03 +41 26 50.8 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347637268576283904,2461093.6803,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347637268576283904 20260222.1803 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:40.03 +41:26:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.05 01:40:10.42 +50:40:29.6
130.77523 -11.45318 galactic Per Second-epoch detections are separated by 7.8" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405811226210751872 | 01:40:10.93 +50:40:26.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 10.42 +50 40 29.6 13.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405811226210751872,2461093.6803,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405811226210751872 20260222.1803 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:10.42 +50:40:29.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.20 01:38:44.76 +49:37:45.6
130.74794 -12.52312 galactic And Second-epoch detections are separated by 2.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405648223611775104 | 01:38:45.34 +49:37:47.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 44.76 +49 37 45.6 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405648223611775104,2461093.6803,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405648223611775104 20260222.1803 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:44.76 +49:37:45.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.24 01:45:52.22 +48:57:57.0
132.05105 -12.93973 galactic And Second-epoch detections are separated by 4.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.4705+48.9662 | 01:45:52.92 +48:57:58.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 52.22 +48 57 57.0 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.4705+48.9662,2461093.6803,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.4705+48.9662 20260222.1803 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:52.22 +48:57:57.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.17 01:43:32.43 +50:24:35.3
131.36395 -11.60697 galactic And Second-epoch detections are separated by 1.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405965428418940672 | 01:43:33.57 +50:24:32.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A1IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 32.43 +50 24 35.3 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405965428418940672,2461093.6803,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405965428418940672 20260222.1803 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:32.43 +50:24:35.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.17 01:37:31.29 +50:24:10.9
130.40436 -11.79890 galactic And Second-epoch detections are separated by 5.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J013727.84+502345.3 | 01:37:27.84 +50:23:45.2 (Gaia DR3) | SRS (local) | 20.525000000000 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 37 31.29 +50 24 10.9 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J013727.84+502345.3,2461093.6803,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J013727.84+502345.3 20260222.1803 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:37:31.29 +50:24:10.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.17 01:45:33.11 +50:14:55.2
131.71882 -11.69757 galactic And Second-epoch detections are separated by 2.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.3802+50.2381 | 01:45:34.27 +50:14:52.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 33.11 +50 14 55.2 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.3802+50.2381,2461093.6803,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.3802+50.2381 20260222.1803 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:33.11 +50:14:55.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.09 01:46:42.32 +50:10:12.3
131.92014 -11.73467 galactic And Second-epoch detections are separated by 5.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405902756256760192 | 01:46:43.02 +50:10:09.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 42.32 +50 10 12.3 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405902756256760192,2461093.6803,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405902756256760192 20260222.1803 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:42.32 +50:10:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.24 01:44:12.08 +42:09:50.1
133.27831 -19.64535 galactic And Second-epoch detections are separated by 7.6" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347737903952039040 | 01:44:12.74 +42:09:55.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 12.08 +42 09 50.1 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347737903952039040,2461093.6803,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347737903952039040 20260222.1803 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:12.08 +42:09:50.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.24 01:42:46.71 +48:02:54.1
131.73360 -13.94405 galactic And Second-epoch detections are separated by 4.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.7108+48.0461 | 01:42:47.50 +48:02:54.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 46.71 +48 02 54.1 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.7108+48.0461,2461093.6803,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.7108+48.0461 20260222.1803 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:46.71 +48:02:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.27 01:47:07.49 +41:16:33.6
134.05426 -20.38997 galactic And Second-epoch detections are separated by 5.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347449904923669376 | 01:47:08.27 +41:16:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 07.49 +41 16 33.6 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347449904923669376,2461093.6803,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347449904923669376 20260222.1803 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:07.49 +41:16:33.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.26 01:45:53.14 +49:31:40.4
131.92990 -12.39024 galactic And Second-epoch detections are separated by 2.2" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405503122437237248 | 01:45:54.05 +49:31:41.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 53.14 +49 31 40.4 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405503122437237248,2461093.6803,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405503122437237248 20260222.1803 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:53.14 +49:31:40.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.14 01:48:01.76 +49:58:50.0
132.17439 -11.87290 galactic Per Second-epoch detections are separated by 2.3" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357858706625029376 | 01:48:02.48 +49:58:52.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 01.76 +49 58 50.0 13.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357858706625029376,2461093.6803,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357858706625029376 20260222.1803 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:01.76 +49:58:50.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.15 01:41:34.03 +47:35:43.1
131.62236 -14.42879 galactic And Second-epoch detections are separated by 8.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399281226653717632 | 01:41:34.67 +47:35:46.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 34.03 +47 35 43.1 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399281226653717632,2461093.6803,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399281226653717632 20260222.1803 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:34.03 +47:35:43.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.12 01:39:11.47 +49:22:07.7
130.87085 -12.76544 galactic And Second-epoch detections are separated by 7.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.8107+49.3677 | 01:39:12.11 +49:22:05.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 11.47 +49 22 07.7 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.8107+49.3677,2461093.6803,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.8107+49.3677 20260222.1803 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:11.47 +49:22:07.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.31 01:46:23.83 +50:05:58.0
131.88652 -11.81432 galactic And Second-epoch detections are separated by 4.8" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:46:23.83 +50:05:58.0 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 23.83 +50 05 58.0 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:23.83 +50:05:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.18 01:41:39.17 +46:45:57.0
131.80869 -15.23860 galactic And Second-epoch detections are separated by 8.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351110518432671232 | 01:41:40.05 +46:45:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 39.17 +46 45 57.0 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351110518432671232,2461093.6803,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351110518432671232 20260222.1803 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:39.17 +46:45:57.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 16.29 +49 36 44.0 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405648739007858944,2461093.6803,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405648739007858944 20260222.1803 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:16.29 +49:36:44.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.27 01:39:11.32 +47:26:23.9
131.24670 -14.65940 galactic And Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399194330875196288 | 01:39:11.93 +47:26:24.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 11.32 +47 26 23.9 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399194330875196288,2461093.6803,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399194330875196288 20260222.1803 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:11.32 +47:26:23.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.22 01:41:39.83 +43:15:07.9
132.55394 -18.67920 galactic And Second-epoch detections are separated by 2.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.4197+43.2530 | 01:41:40.75 +43:15:10.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 39.83 +43 15 07.9 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.4197+43.2530,2461093.6803,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.4197+43.2530 20260222.1803 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:39.83 +43:15:07.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.19 01:41:47.04 +42:49:16.7
132.66990 -19.09647 galactic And Second-epoch detections are separated by 5.2" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348624355140132096 | 01:41:48.15 +42:49:21.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 47.04 +42 49 16.7 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348624355140132096,2461093.6803,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348624355140132096 20260222.1803 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:47.04 +42:49:16.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.09 01:43:57.46 +44:22:08.2
132.73526 -17.50079 galactic And Second-epoch detections are separated by 5.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350221979895397888 | 01:43:58.22 +44:22:10.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 57.46 +44 22 08.2 13.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350221979895397888,2461093.6803,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350221979895397888 20260222.1803 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:57.46 +44:22:08.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.36 01:40:01.06 +46:44:49.1
131.52793 -15.31235 galactic And Second-epoch detections are separated by 3.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351101589196821888 | 01:40:02.17 +46:44:49.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 01.06 +46 44 49.1 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351101589196821888,2461093.6803,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351101589196821888 20260222.1803 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:01.06 +46:44:49.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.34 01:45:23.80 +41:52:27.9
133.57566 -19.87944 galactic And Second-epoch detections are separated by 3.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347683619863263744 | 01:45:24.70 +41:52:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 23.80 +41 52 27.9 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347683619863263744,2461093.6803,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347683619863263744 20260222.1803 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:23.80 +41:52:27.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.17 01:47:39.04 +41:09:46.3
134.18468 -20.47739 galactic And Second-epoch detections are separated by 4.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347401354612815872 | 01:47:39.61 +41:09:51.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 39.04 +41 09 46.3 13.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347401354612815872,2461093.6803,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347401354612815872 20260222.1803 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:39.04 +41:09:46.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.28 01:42:35.62 +43:19:12.3
132.71392 -18.57790 galactic And Second-epoch detections are separated by 5.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348660566006481024 | 01:42:36.46 +43:19:18.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 35.62 +43 19 12.3 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348660566006481024,2461093.6803,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348660566006481024 20260222.1803 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:35.62 +43:19:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.28 01:41:34.81 +50:04:10.2
131.12020 -12.00336 galactic And Second-epoch detections are separated by 8.1" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405592870073261312 | 01:41:35.45 +50:04:11.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 34.81 +50 04 10.2 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405592870073261312,2461093.6803,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405592870073261312 20260222.1803 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:34.81 +50:04:10.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 47.62 +47 52 24.7 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357264042632701056,2461093.6803,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357264042632701056 20260222.1803 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:47.62 +47:52:24.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.38 01:45:47.96 +50:04:49.7
131.79500 -11.85345 galactic And Second-epoch detections are separated by 2.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405907364759625472 | 01:45:49.07 +50:04:50.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 47.96 +50 04 49.7 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405907364759625472,2461093.6803,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405907364759625472 20260222.1803 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:47.96 +50:04:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.48 01:45:14.42 +49:04:08.3
131.92493 -12.86104 galactic And Second-epoch detections are separated by 5.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.2978+49.0701 | 01:45:15.10 +49:04:06.7 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 14.42 +49 04 08.3 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.2978+49.0701,2461093.6803,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.2978+49.0701 20260222.1803 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:14.42 +49:04:08.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.31 01:46:04.17 +42:10:40.0
133.63358 -19.55591 galactic And Second-epoch detections are separated by 6.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 347782369751197696 | 01:46:04.56 +42:10:46.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 04.17 +42 10 40.0 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 347782369751197696,2461093.6803,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 347782369751197696 20260222.1803 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:04.17 +42:10:40.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.29 01:40:10.03 +47:23:35.8
131.42389 -14.67340 galactic And Second-epoch detections are separated by 8.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399182197591045760 | 01:40:10.70 +47:23:36.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 10.03 +47 23 35.8 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399182197591045760,2461093.6803,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399182197591045760 20260222.1803 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:10.03 +47:23:35.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.50 01:45:15.59 +49:25:52.2
131.84932 -12.50642 galactic And Second-epoch detections are separated by 4.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405501404450978816 | 01:45:16.57 +49:25:53.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 15.59 +49 25 52.2 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405501404450978816,2461093.6803,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405501404450978816 20260222.1803 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:15.59 +49:25:52.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.42 01:43:55.65 +43:11:05.6
132.99450 -18.65893 galactic And Second-epoch detections are separated by 4.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348644799184502528 | 01:43:56.78 +43:11:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 55.65 +43 11 05.6 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348644799184502528,2461093.6803,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348644799184502528 20260222.1803 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:55.65 +43:11:05.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.38 01:51:13.71 +50:00:48.0
132.67809 -11.72357 galactic Per Second-epoch detections are separated by 6.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357824548748861056 | 01:51:14.34 +50:00:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 51 13.71 +50 00 48.0 13.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357824548748861056,2461093.6803,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357824548748861056 20260222.1803 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:13.71 +50:00:48.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.29 01:43:08.01 +41:05:22.5
133.31587 -20.73749 galactic And Second-epoch detections are separated by 6.3" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347251133836057344 | 01:43:08.41 +41:05:28.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 08.01 +41 05 22.5 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347251133836057344,2461093.6803,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347251133836057344 20260222.1803 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:08.01 +41:05:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.38 01:40:26.75 +50:42:36.7
130.81146 -11.41025 galactic Per Second-epoch detections are separated by 1.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406186262755235840 | 01:40:27.40 +50:42:33.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 26.75 +50 42 36.7 13.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406186262755235840,2461093.6803,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406186262755235840 20260222.1803 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:26.75 +50:42:36.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 52.27 +49 43 52.5 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405654850745584896,2461093.6803,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405654850745584896 20260222.1803 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:52.27 +49:43:52.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.52 01:41:22.02 +43:22:47.8
132.47072 -18.56512 galactic And Second-epoch detections are separated by 6.9" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348688740991938048 | 01:41:23.18 +43:22:51.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 22.02 +43 22 47.8 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348688740991938048,2461093.6803,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348688740991938048 20260222.1803 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:22.02 +43:22:47.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.47 01:41:51.87 +44:47:41.4
132.26070 -17.16157 galactic And Second-epoch detections are separated by 6.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350292481780586368 | 01:41:52.58 +44:47:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 51.87 +44 47 41.4 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350292481780586368,2461093.6803,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350292481780586368 20260222.1803 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:51.87 +44:47:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.47 01:45:00.36 +50:35:25.7
131.55832 -11.38188 galactic And Second-epoch detections are separated by 4.1" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405993813860839808 | 01:45:01.35 +50:35:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 00.36 +50 35 25.7 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405993813860839808,2461093.6803,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405993813860839808 20260222.1803 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:00.36 +50:35:25.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.51 01:41:52.74 +48:30:11.1
131.48824 -13.52888 galactic And Second-epoch detections are separated by 4.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405344204349255168 | 01:41:53.19 +48:30:06.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 52.74 +48 30 11.1 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405344204349255168,2461093.6803,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405344204349255168 20260222.1803 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:52.74 +48:30:11.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.36 01:41:09.12 +50:32:09.1
130.95811 -11.55953 galactic And Second-epoch detections are separated by 3.6" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.2956+50.5346 | 01:41:10.95 +50:32:04.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 09.12 +50 32 09.1 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.2956+50.5346,2461093.6803,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.2956+50.5346 20260222.1803 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:09.12 +50:32:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.41 01:45:13.52 +50:03:38.4
131.70733 -11.89238 galactic And Second-epoch detections are separated by 1.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405906608845067648 | 01:45:14.82 +50:03:39.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 13.52 +50 03 38.4 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405906608845067648,2461093.6803,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405906608845067648 20260222.1803 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:13.52 +50:03:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.43 01:41:16.39 +50:02:34.2
131.07617 -12.03921 galactic And Second-epoch detections are separated by 3.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405592590898633216 | 01:41:17.20 +50:02:33.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 16.39 +50 02 34.2 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405592590898633216,2461093.6803,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405592590898633216 20260222.1803 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:16.39 +50:02:34.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.45 01:45:44.25 +48:18:31.2
132.17411 -13.58627 galactic And Second-epoch detections are separated by 2.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357299428866871040 | 01:45:44.87 +48:18:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 44.25 +48 18 31.2 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357299428866871040,2461093.6803,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357299428866871040 20260222.1803 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:44.25 +48:18:31.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.47 01:43:03.73 +50:33:40.0
131.25645 -11.47435 galactic And Second-epoch detections are separated by 1.9" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405979176612314880 | 01:43:04.69 +50:33:39.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.626+/-0.171 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 03.73 +50 33 40.0 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405979176612314880,2461093.6803,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405979176612314880 20260222.1803 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:03.73 +50:33:40.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.36 01:46:28.14 +49:35:08.9
132.01169 -12.31330 galactic And Second-epoch detections are separated by 3.2" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357470922617469568 | 01:46:29.24 +49:35:06.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 28.14 +49 35 08.9 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357470922617469568,2461093.6803,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357470922617469568 20260222.1803 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:28.14 +49:35:08.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.37 01:45:55.88 +50:44:39.8
131.67117 -11.20038 galactic Per Second-epoch detections are separated by 5.9" and 5.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406001849742237312 | 01:45:56.49 +50:44:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 55.88 +50 44 39.8 13.4 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406001849742237312,2461093.6803,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406001849742237312 20260222.1803 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:55.88 +50:44:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.41 01:42:35.85 +41:06:58.6
133.20431 -20.73278 galactic And Second-epoch detections are separated by 5.0" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347262227734073600 | 01:42:36.68 +41:07:03.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 35.85 +41 06 58.6 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347262227734073600,2461093.6803,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347262227734073600 20260222.1803 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:35.85 +41:06:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.61 01:50:37.60 +50:34:55.7
132.44745 -11.19283 galactic Per Second-epoch detections are separated by 3.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357994388934173696 | 01:50:38.60 +50:34:52.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 50 37.60 +50 34 55.7 13.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357994388934173696,2461093.6803,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357994388934173696 20260222.1803 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:50:37.60 +50:34:55.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.43 01:39:43.63 +46:42:23.2
131.48542 -15.36175 galactic And Second-epoch detections are separated by 1.0" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351095778104904320 | 01:39:44.66 +46:42:22.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 43.63 +46 42 23.2 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351095778104904320,2461093.6803,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351095778104904320 20260222.1803 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:43.63 +46:42:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.43 01:41:31.88 +43:16:12.5
132.52515 -18.66655 galactic And Second-epoch detections are separated by 7.3" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348639439065142016 | 01:41:32.54 +43:16:17.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 31.88 +43 16 12.5 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348639439065142016,2461093.6803,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348639439065142016 20260222.1803 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:31.88 +43:16:12.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.29 01:41:29.77 +42:45:16.0
132.62967 -19.17272 galactic And Second-epoch detections are separated by 7.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348530102079875584 | 01:41:30.40 +42:45:19.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 29.77 +42 45 16.0 13.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348530102079875584,2461093.6803,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348530102079875584 20260222.1803 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:29.77 +42:45:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.64 01:41:46.39 +44:21:09.3
132.33825 -17.59789 galactic And Second-epoch detections are separated by 4.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350254174969854464 | 01:41:46.95 +44:21:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 46.39 +44 21 09.3 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350254174969854464,2461093.6803,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350254174969854464 20260222.1803 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:46.39 +44:21:09.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.52 01:43:12.02 +50:32:39.7
131.28185 -11.48629 galactic And Second-epoch detections are separated by 2.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405984772951639296 | 01:43:12.82 +50:32:36.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A7V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 12.02 +50 32 39.7 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405984772951639296,2461093.6803,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405984772951639296 20260222.1803 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:12.02 +50:32:39.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.52 01:43:58.52 +47:40:24.8
132.01583 -14.26941 galactic And Second-epoch detections are separated by 4.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 351258849422554112 | 01:43:59.43 +47:40:25.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 58.52 +47 40 24.8 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 351258849422554112,2461093.6803,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 351258849422554112 20260222.1803 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:58.52 +47:40:24.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.69 01:46:25.78 +41:40:10.5
133.82399 -20.03617 galactic And Second-epoch detections are separated by 5.5" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347478487928319872 | 01:46:26.40 +41:40:20.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 25.78 +41 40 10.5 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347478487928319872,2461093.6803,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347478487928319872 20260222.1803 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:25.78 +41:40:10.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.57 01:40:20.90 +50:28:37.1
130.84180 -11.64209 galactic And Second-epoch detections are separated by 6.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405795970486957184 | 01:40:21.95 +50:28:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 20.90 +50 28 37.1 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405795970486957184,2461093.6803,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405795970486957184 20260222.1803 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:20.90 +50:28:37.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.45 01:44:34.81 +42:55:59.7
133.17454 -18.87910 galactic And Second-epoch detections are separated by 2.2" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347887166952894080 | 01:44:35.38 +42:56:07.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 34.81 +42 55 59.7 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347887166952894080,2461093.6803,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347887166952894080 20260222.1803 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:34.81 +42:55:59.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.59 01:46:00.65 +50:03:46.1
131.83273 -11.86344 galactic And Second-epoch detections are separated by 2.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405895575071445504 | 01:46:01.87 +50:03:44.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 00.65 +50 03 46.1 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405895575071445504,2461093.6803,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405895575071445504 20260222.1803 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:00.65 +50:03:46.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.42 01:41:56.25 +42:44:53.5
132.71498 -19.16222 galactic And Second-epoch detections are separated by 7.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348518355347063936 | 01:41:56.76 +42:44:58.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 56.25 +42 44 53.5 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348518355347063936,2461093.6803,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348518355347063936 20260222.1803 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:56.25 +42:44:53.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 22 26.91 +42 18 07.3 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:22:26.91 +42:18:07.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.65 01:42:40.09 +41:50:36.9
133.05494 -20.01896 galactic And Second-epoch detections are separated by 6.3" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.6732+41.8481 | 01:42:40.96 +41:50:40.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 40.09 +41 50 36.9 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.6732+41.8481,2461093.6803,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.6732+41.8481 20260222.1803 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:40.09 +41:50:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.56 01:44:48.28 +40:57:58.0
133.67352 -20.78988 galactic And Second-epoch detections are separated by 3.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.1961+40.9653 | 01:44:48.76 +40:58:03.2 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 48.28 +40 57 58.0 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.1961+40.9653,2461093.6803,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.1961+40.9653 20260222.1803 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:48.28 +40:57:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.61 01:38:10.39 +50:22:34.6
130.51368 -11.80621 galactic And Second-epoch detections are separated by 8.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.5419+50.3700 | 01:38:10.88 +50:22:30.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 10.39 +50 22 34.6 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.5419+50.3700,2461093.6803,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.5419+50.3700 20260222.1803 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:10.39 +50:22:34.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.56 01:47:13.39 +50:08:57.4
132.00744 -11.73688 galactic And Second-epoch detections are separated by 5.9" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.8070+50.1518 | 01:47:14.32 +50:08:58.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 13.39 +50 08 57.4 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.8070+50.1518,2461093.6803,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.8070+50.1518 20260222.1803 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:13.39 +50:08:57.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.73 01:42:02.91 +41:38:42.5
132.97869 -20.23717 galactic And Second-epoch detections are separated by 5.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.5134+41.6470 | 01:42:03.23 +41:38:49.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 02.91 +41 38 42.5 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.5134+41.6470,2461093.6803,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.5134+41.6470 20260222.1803 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:02.91 +41:38:42.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.57 01:41:20.24 +49:23:44.2
131.21690 -12.67175 galactic And Second-epoch detections are separated by 0.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405445398076178304 | 01:41:20.81 +49:23:46.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 20.24 +49 23 44.2 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405445398076178304,2461093.6803,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405445398076178304 20260222.1803 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:20.24 +49:23:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.62 01:41:40.64 +50:38:38.2
131.01986 -11.43717 galactic Per Second-epoch detections are separated by 1.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406170281180843520 | 01:41:41.40 +50:38:37.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 40.64 +50 38 38.2 13.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406170281180843520,2461093.6803,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406170281180843520 20260222.1803 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:40.64 +50:38:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 40.73 +49 57 41.8 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:40.73 +49:57:41.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.70 01:56:48.56 +43:10:17.5
135.40110 -18.11185 galactic And Second-epoch detections are separated by 3.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:56:48.56 +43:10:17.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 56 48.56 +43 10 17.5 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:56:48.56 +43:10:17.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.74 01:40:26.67 +49:25:27.3
131.06518 -12.67203 galactic And Second-epoch detections are separated by 6.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405457625847786496 | 01:40:28.16 +49:25:30.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 26.67 +49 25 27.3 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405457625847786496,2461093.6803,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405457625847786496 20260222.1803 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:26.67 +49:25:27.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.62 01:42:45.77 +42:01:56.6
133.03106 -19.83067 galactic And Second-epoch detections are separated by 5.5" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347721587373995136 | 01:42:46.43 +42:01:57.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 45.77 +42 01 56.6 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347721587373995136,2461093.6803,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347721587373995136 20260222.1803 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:45.77 +42:01:56.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.62 01:41:05.23 +44:36:05.5
132.15988 -17.37878 galactic And Second-epoch detections are separated by 6.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350448062676530560 | 01:41:05.74 +44:36:13.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 05.23 +44 36 05.5 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350448062676530560,2461093.6803,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350448062676530560 20260222.1803 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:05.23 +44:36:05.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.68 01:48:38.44 +50:20:15.2
132.19044 -11.50305 galactic Per Second-epoch detections are separated by 8.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357892855909687168 | 01:48:39.31 +50:20:14.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 38.44 +50 20 15.2 13.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357892855909687168,2461093.6803,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357892855909687168 20260222.1803 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:38.44 +50:20:15.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.68 01:44:30.20 +50:39:18.1
131.46502 -11.33543 galactic Per Second-epoch detections are separated by 1.9" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:44:30.20 +50:39:18.1 (user input) | T | P | (position from user input) SpType: A5V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 30.20 +50 39 18.1 13.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:30.20 +50:39:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.62 01:45:34.46 +49:47:07.4
131.82320 -12.14946 galactic And Second-epoch detections are separated by 8.1" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405516522735152384 | 01:45:35.18 +49:47:08.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 34.46 +49 47 07.4 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405516522735152384,2461093.6803,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405516522735152384 20260222.1803 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:34.46 +49:47:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 44.88 +50 12 26.3 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405598913090485504,2461093.6803,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405598913090485504 20260222.1803 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:44.88 +50:12:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.61 01:41:52.77 +44:11:18.7
132.39288 -17.75463 galactic And Second-epoch detections are separated by 6.8" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350239808301704448 | 01:41:53.58 +44:11:19.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 52.77 +44 11 18.7 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350239808301704448,2461093.6803,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350239808301704448 20260222.1803 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:52.77 +44:11:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.53 01:48:45.20 +50:33:06.6
132.15921 -11.29021 galactic Per Second-epoch detections are separated by 4.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J027.1777+50.5598 | 01:48:46.01 +50:33:04.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 45.20 +50 33 06.6 13.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J027.1777+50.5598,2461093.6803,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J027.1777+50.5598 20260222.1803 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:45.20 +50:33:06.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.62 01:54:13.09 +50:55:58.7
132.92413 -10.71672 galactic Per Second-epoch detections are separated by 8.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:54:13.09 +50:55:58.7 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5) J-Ks=0.707+/-0.676 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 54 13.09 +50 55 58.7 13.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:54:13.09 +50:55:58.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.75 01:42:51.48 +50:52:29.6
131.15942 -11.17360 galactic Per Second-epoch detections are separated by 0.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406203580064051584 | 01:42:52.36 +50:52:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 51.48 +50 52 29.6 13.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406203580064051584,2461093.6803,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406203580064051584 20260222.1803 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:51.48 +50:52:29.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.77 02:18:18.35 +49:53:11.9
136.96884 -10.60273 galactic And Second-epoch detections are separated by 0.7" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J034.5798+49.8980 | 02:18:18.35 +49:53:11.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 18 18.35 +49 53 11.9 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J034.5798+49.8980,2461093.6803,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J034.5798+49.8980 20260222.1803 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:18:18.35 +49:53:11.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 38.46 +41 34 18.3 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347476705519406080,2461093.6803,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347476705519406080 20260222.1803 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:38.46 +41:34:18.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.83 01:40:33.18 +49:47:52.3
131.00874 -12.30209 galactic And Second-epoch detections are separated by 2.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405560533262721664 | 01:40:33.87 +49:47:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 33.18 +49 47 52.3 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405560533262721664,2461093.6803,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405560533262721664 20260222.1803 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:33.18 +49:47:52.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.82 01:39:04.13 +49:43:21.1
130.78259 -12.42179 galactic And Second-epoch detections are separated by 3.6" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405656091991825024 | 01:39:04.76 +49:43:21.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 04.13 +49 43 21.1 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405656091991825024,2461093.6803,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405656091991825024 20260222.1803 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:04.13 +49:43:21.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.71 01:45:11.61 +49:46:13.1
131.76502 -12.17726 galactic And Second-epoch detections are separated by 3.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:45:11.61 +49:46:13.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 11.61 +49 46 13.1 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:11.61 +49:46:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.68 01:45:19.00 +42:29:43.3
133.41520 -19.27699 galactic And Second-epoch detections are separated by 2.9" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347842151403477376 | 01:45:19.69 +42:29:45.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 19.00 +42 29 43.3 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347842151403477376,2461093.6803,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347842151403477376 20260222.1803 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:19.00 +42:29:43.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 53.36 +41 42 06.2 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:53.36 +41:42:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.66 01:42:24.83 +43:21:44.5
132.67093 -18.54333 galactic And Second-epoch detections are separated by 3.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348661394937929088 | 01:42:26.09 +43:21:44.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 24.83 +43 21 44.5 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348661394937929088,2461093.6803,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348661394937929088 20260222.1803 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:24.83 +43:21:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.84 01:39:29.18 +50:16:33.7
130.74318 -11.86557 galactic And Second-epoch detections are separated by 6.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405775419067231488 | 01:39:29.81 +50:16:31.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 29.18 +50 16 33.7 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405775419067231488,2461093.6803,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405775419067231488 20260222.1803 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:29.18 +50:16:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.84 01:53:01.77 +50:59:18.7
132.72561 -10.70827 galactic Per Second-epoch detections are separated by 4.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 359515601929305088 | 01:53:02.46 +50:59:15.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 53 01.77 +50 59 18.7 13.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 359515601929305088,2461093.6803,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 359515601929305088 20260222.1803 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:53:01.77 +50:59:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.72 01:41:41.33 +49:43:08.2
131.20869 -12.34353 galactic And Second-epoch detections are separated by 6.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405561495335428608 | 01:41:42.25 +49:43:08.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 41.33 +49 43 08.2 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405561495335428608,2461093.6803,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405561495335428608 20260222.1803 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:41.33 +49:43:08.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.64 01:43:37.79 +43:49:53.3
132.79431 -18.03854 galactic And Second-epoch detections are separated by 6.2" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350175693029517312 | 01:43:38.54 +43:49:57.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 37.79 +43 49 53.3 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350175693029517312,2461093.6803,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350175693029517312 20260222.1803 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:37.79 +43:49:53.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 27.48 +50 28 06.0 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405977763565013376,2461093.6803,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405977763565013376 20260222.1803 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:27.48 +50:28:06.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.87 01:43:11.97 +44:52:32.4
132.48560 -17.03375 galactic And Second-epoch detections are separated by 6.4" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:43:11.97 +44:52:32.4 (user input) | T | P | (position from user input) SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 11.97 +44 52 32.4 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:11.97 +44:52:32.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.65 01:46:10.95 +49:00:54.1
132.09148 -12.88066 galactic And Second-epoch detections are separated by 5.7" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 357429759651071872 | 01:46:11.64 +49:00:55.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 10.95 +49 00 54.1 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357429759651071872,2461093.6803,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357429759651071872 20260222.1803 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:10.95 +49:00:54.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.86 01:38:20.74 +50:37:24.7
130.49466 -11.55814 galactic And Second-epoch detections are separated by 7.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405853553115529472 | 01:38:21.22 +50:37:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 20.74 +50 37 24.7 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405853553115529472,2461093.6803,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405853553115529472 20260222.1803 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:20.74 +50:37:24.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.70 01:46:28.51 +49:52:23.4
131.94903 -12.03254 galactic And Second-epoch detections are separated by 4.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405890287969727360 | 01:46:29.24 +49:52:23.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 28.51 +49 52 23.4 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405890287969727360,2461093.6803,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405890287969727360 20260222.1803 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:28.51 +49:52:23.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.73 01:41:32.61 +49:02:41.5
131.32182 -13.00894 galactic And Second-epoch detections are separated by 5.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405431787322389120 | 01:41:33.32 +49:02:40.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 32.61 +49 02 41.5 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405431787322389120,2461093.6803,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405431787322389120 20260222.1803 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:32.61 +49:02:41.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.88 01:44:12.76 +41:15:28.4
133.48916 -20.52948 galactic And Second-epoch detections are separated by 4.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347628369404081536 | 01:44:13.32 +41:15:32.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 12.76 +41 15 28.4 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347628369404081536,2461093.6803,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347628369404081536 20260222.1803 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:12.76 +41:15:28.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.88 01:42:25.29 +41:30:33.2
133.08166 -20.35555 galactic And Second-epoch detections are separated by 7.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347693378028870272 | 01:42:25.98 +41:30:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 25.29 +41 30 33.2 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347693378028870272,2461093.6803,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347693378028870272 20260222.1803 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:25.29 +41:30:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.76 01:41:32.23 +45:53:25.1
131.97086 -16.10033 galactic And Second-epoch detections are separated by 4.5" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350637247395016960 | 01:41:33.56 +45:53:26.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 32.23 +45 53 25.1 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350637247395016960,2461093.6803,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350637247395016960 20260222.1803 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:32.23 +45:53:25.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.69 01:45:22.30 +49:57:25.0
131.75327 -11.98877 galactic And Second-epoch detections are separated by 5.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405904925217899904 | 01:45:23.04 +49:57:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 22.30 +49 57 25.0 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405904925217899904,2461093.6803,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405904925217899904 20260222.1803 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:22.30 +49:57:25.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.86 01:39:38.57 +48:18:37.7
131.15247 -13.79036 galactic And Second-epoch detections are separated by 2.7" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399380491937585024 | 01:39:39.71 +48:18:37.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 38.57 +48 18 37.7 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399380491937585024,2461093.6803,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399380491937585024 20260222.1803 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:38.57 +48:18:37.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.86 01:49:03.79 +41:05:49.8
134.47713 -20.47915 galactic And Second-epoch detections are separated by 1.3" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347391527727849984 | 01:49:04.43 +41:05:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 49 03.79 +41 05 49.8 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347391527727849984,2461093.6803,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347391527727849984 20260222.1803 13.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:49:03.79 +41:05:49.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 20.89 +48 05 07.4 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399326645930390784,2461093.6803,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399326645930390784 20260222.1803 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:20.89 +48:05:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.79 01:52:01.75 +50:43:20.4
132.63421 -11.00445 galactic Per Second-epoch detections are separated by 6.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 358005147830086144 | 01:52:02.43 +50:43:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 52 01.75 +50 43 20.4 13.8 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 358005147830086144,2461093.6803,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 358005147830086144 20260222.1803 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:52:01.75 +50:43:20.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 27.45 +49 45 10.3 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:27.45 +49:45:10.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 02.95 +50 49 28.9 14.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:02.95 +50:49:28.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.87 01:47:18.94 +49:50:41.9
132.09048 -12.03052 galactic And Second-epoch detections are separated by 6.1" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.7943+49.8359 | 01:47:14.45 +49:50:30.1 (Gaia DR3) | NSINE (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 18.94 +49 50 41.9 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.7943+49.8359,2461093.6803,13.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.7943+49.8359 20260222.1803 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:18.94 +49:50:41.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.90 01:42:20.08 +50:49:16.0
131.08794 -11.24287 galactic Per Second-epoch detections are separated by 5.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406179730112131200 | 01:42:20.84 +50:49:15.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 20.08 +50 49 16.0 13.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406179730112131200,2461093.6803,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406179730112131200 20260222.1803 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:20.08 +50:49:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.82 01:43:23.89 +42:07:14.2
133.13371 -19.71953 galactic And Second-epoch detections are separated by 4.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347735258252185856 | 01:43:24.58 +42:07:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 23.89 +42 07 14.2 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347735258252185856,2461093.6803,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347735258252185856 20260222.1803 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:23.89 +42:07:14.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 43.91 +48 34 01.6 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:43.91 +48:34:01.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.88 01:39:18.03 +48:11:10.5
131.11925 -13.92317 galactic And Second-epoch detections are separated by 2.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399355443688349568 | 01:39:18.56 +48:11:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 18.03 +48 11 10.5 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399355443688349568,2461093.6803,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399355443688349568 20260222.1803 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:18.03 +48:11:10.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 18.98 +50 21 32.1 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:18.98 +50:21:32.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.94 01:44:27.99 +50:36:09.1
131.47035 -11.38800 galactic And Second-epoch detections are separated by 0.5" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.1192+50.6023 | 01:44:28.63 +50:36:08.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 27.99 +50 36 09.1 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.1192+50.6023,2461093.6803,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.1192+50.6023 20260222.1803 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:27.99 +50:36:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 47.48 +40 55 31.0 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347423688442819584,2461093.6803,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347423688442819584 20260222.1803 13.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:47.48 +40:55:31.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.95 01:41:34.51 +50:12:58.6
131.08978 -11.85963 galactic And Second-epoch detections are separated by 6.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405596129951677184 | 01:41:35.22 +50:12:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 34.51 +50 12 58.6 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405596129951677184,2461093.6803,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405596129951677184 20260222.1803 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:34.51 +50:12:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.10 01:40:19.08 +50:48:57.1
130.77049 -11.31045 galactic Per Second-epoch detections are separated by 3.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 406187942086359296 | 01:40:19.41 +50:49:02.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 19.08 +50 48 57.1 14.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 406187942086359296,2461093.6803,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 406187942086359296 20260222.1803 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:19.08 +50:48:57.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 41.87 +40 50 33.1 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:41.87 +40:50:33.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 06.04 +49 51 07.1 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:06.04 +49:51:07.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 48 01.18 +40 58 04.6 13.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:48:01.18 +40:58:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.15 01:37:53.96 +49:36:12.5
130.61479 -12.57393 galactic And Second-epoch detections are separated by 8.0" and 6.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405658978209895808 | 01:37:54.84 +49:36:15.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 37 53.96 +49 36 12.5 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405658978209895808,2461093.6803,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405658978209895808 20260222.1803 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:37:53.96 +49:36:12.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.05 01:39:22.89 +49:33:38.1
130.86481 -12.57127 galactic And Second-epoch detections are separated by 4.3" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J024.8335+49.5588 | 01:39:22.89 +49:33:38.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 22.89 +49 33 38.1 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J024.8335+49.5588,2461093.6803,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J024.8335+49.5588 20260222.1803 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:22.89 +49:33:38.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 59.00 +49 23 43.8 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:59.00 +49:23:43.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.01 01:44:27.15 +41:10:32.2
133.55528 -20.59998 galactic And Second-epoch detections are separated by 4.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347624246235486464 | 01:44:27.99 +41:10:40.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 27.15 +41 10 32.2 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347624246235486464,2461093.6803,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347624246235486464 20260222.1803 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:27.15 +41:10:32.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.21 01:38:20.35 +50:37:01.3
130.49485 -11.56472 galactic And Second-epoch detections are separated by 1.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405853553115529472 | 01:38:21.22 +50:37:16.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 20.35 +50 37 01.3 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405853553115529472,2461093.6803,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405853553115529472 20260222.1803 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:20.35 +50:37:01.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.08 01:40:13.36 +49:51:56.8
130.94183 -12.24573 galactic And Second-epoch detections are separated by 5.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.0618+49.8814 | 01:40:14.83 +49:52:08.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 13.36 +49 51 56.8 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.0618+49.8814,2461093.6803,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.0618+49.8814 20260222.1803 14.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:13.36 +49:51:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 17.75 +50 48 53.9 14.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:17.75 +50:48:53.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 15.98 +49 06 39.2 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:15.98 +49:06:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.01 01:40:30.40 +47:19:17.1
131.49667 -14.73268 galactic And Second-epoch detections are separated by 8.5" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399178800273496448 | 01:40:31.06 +47:19:18.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 30.40 +47 19 17.1 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399178800273496448,2461093.6803,14.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399178800273496448 20260222.1803 14.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:30.40 +47:19:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 46.17 +41 07 25.0 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:46.17 +41:07:25.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 58.19 +41 00 40.6 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:58.19 +41:00:40.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.08 01:44:32.18 +50:29:57.3
131.50337 -11.48670 galactic And Second-epoch detections are separated by 4.4" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:44:32.18 +50:29:57.3 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 32.18 +50 29 57.3 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:32.18 +50:29:57.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 07.56 +40 53 48.6 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:07.56 +40:53:48.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.21 01:39:12.53 +48:41:45.9
131.00434 -13.42548 galactic And Second-epoch detections are separated by 8.0" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399406944638468736 | 01:39:11.99 +48:41:31.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 12.53 +48 41 45.9 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399406944638468736,2461093.6803,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399406944638468736 20260222.1803 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:12.53 +48:41:45.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 07.84 +50 03 45.1 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:07.84 +50:03:45.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 19.09 +42 16 51.5 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:19.09 +42:16:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.06 01:38:11.35 +50:28:56.2
130.49630 -11.70155 galactic And Second-epoch detections are separated by 1.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405828401782331520 | 01:38:11.56 +50:29:02.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 11.35 +50 28 56.2 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405828401782331520,2461093.6803,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405828401782331520 20260222.1803 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:11.35 +50:28:56.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 52.76 +43 11 19.5 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348635281536830208,2461093.6803,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348635281536830208 20260222.1803 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:52.76 +43:11:19.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.11 01:39:50.55 +46:04:05.1
131.63402 -15.98419 galactic And Second-epoch detections are separated by 4.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:39:50.55 +46:04:05.1 (user input) | T | P | (position from user input) SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 50.55 +46 04 05.1 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:50.55 +46:04:05.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.03 01:41:53.55 +49:30:18.0
131.28532 -12.54666 galactic And Second-epoch detections are separated by 7.5" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405540226657392384 | 01:41:54.21 +49:30:15.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 53.55 +49 30 18.0 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405540226657392384,2461093.6803,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405540226657392384 20260222.1803 14.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:53.55 +49:30:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 41.14 +48 13 18.4 14.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:41.14 +48:13:18.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 14.44 +50 19 46.5 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:14.44 +50:19:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.13 01:43:35.00 +50:17:09.0
131.39672 -11.72691 galactic And Second-epoch detections are separated by 3.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:43:35.00 +50:17:09.0 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 35.00 +50 17 09.0 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:35.00 +50:17:09.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 14.37 +40 53 42.7 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:14.37 +40:53:42.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.13 01:46:24.88 +50:22:00.8
131.83035 -11.55258 galactic And Second-epoch detections are separated by 6.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:46:24.88 +50:22:00.8 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 24.88 +50 22 00.8 14.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:24.88 +50:22:00.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.19 01:37:14.74 +50:41:50.2
130.30599 -11.51744 galactic Per Second-epoch detections are separated by 4.5" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 405869358590494208 | 01:37:15.41 +50:41:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 37 14.74 +50 41 50.2 14.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405869358590494208,2461093.6803,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405869358590494208 20260222.1803 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:37:14.74 +50:41:50.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 13.93 +50 12 17.6 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:13.93 +50:12:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 48.98 +42 02 42.4 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:48.98 +42:02:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.32 01:40:06.33 +46:27:55.9
131.60006 -15.58549 galactic And Second-epoch detections are separated by 5.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:40:06.33 +46:27:55.9 (user input) | T | P | (position from user input) SpType: A6IV (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 06.33 +46 27 55.9 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:06.33 +46:27:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.41 01:43:10.86 +49:20:43.3
131.52860 -12.66077 galactic And Second-epoch detections are separated by 4.6" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.7931+49.3395 | 01:43:10.86 +49:20:43.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 10.86 +49 20 43.3 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.7931+49.3395,2461093.6803,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.7931+49.3395 20260222.1803 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:10.86 +49:20:43.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.34 01:41:40.69 +49:13:48.9
131.30626 -12.82286 galactic And Second-epoch detections are separated by 2.9" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:41:40.69 +49:13:48.9 (user input) | T | P | (position from user input) SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 40.69 +49 13 48.9 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:40.69 +49:13:48.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.28 01:42:00.01 +42:10:17.7
132.85319 -19.72403 galactic And Second-epoch detections are separated by 4.6" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:42:00.01 +42:10:17.7 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 00.01 +42 10 17.7 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:00.01 +42:10:17.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 19.84 +41 07 56.5 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:19.84 +41:07:56.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 56.77 +48 16 07.7 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 357279435795609600,2461093.6803,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 357279435795609600 20260222.1803 14.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:56.77 +48:16:07.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 04.56 +40 54 34.9 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347420527346893056,2461093.6803,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347420527346893056 20260222.1803 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:04.56 +40:54:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.31 01:39:21.30 +49:18:05.4
130.91077 -12.82648 galactic And Second-epoch detections are separated by 6.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:39:21.30 +49:18:05.4 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 39 21.30 +49 18 05.4 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:39:21.30 +49:18:05.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.31 01:44:04.71 +50:31:10.7
131.42639 -11.48187 galactic And Second-epoch detections are separated by 7.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J026.0233+50.5190 | 01:44:04.71 +50:31:10.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F2 (LAMOST DR5) J-Ks=1.356+/- (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 04.71 +50 31 10.7 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J026.0233+50.5190,2461093.6803,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J026.0233+50.5190 20260222.1803 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:04.71 +50:31:10.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 47.42 +49 33 53.7 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 405460000964950656,2461093.6803,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 405460000964950656 20260222.1803 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:47.42 +49:33:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 38 12.28 +49 40 34.7 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:38:12.28 +49:40:34.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 31.22 +50 15 16.3 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:31.22 +50:15:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 47 32.15 +41 04 11.7 14.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347399808424612224,2461093.6803,14.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347399808424612224 20260222.1803 14.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:47:32.15 +41:04:11.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.27 01:43:43.30 +41:17:08.3
133.38657 -20.52231 galactic And Second-epoch detections are separated by 8.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.9354+41.2871 | 01:43:43.30 +41:17:08.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 43.30 +41 17 08.3 14.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.9354+41.2871,2461093.6803,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.9354+41.2871 20260222.1803 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:43.30 +41:17:08.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.18 01:42:51.60 +41:39:26.6
133.13392 -20.19346 galactic And Second-epoch detections are separated by 4.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:42:51.60 +41:39:26.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 51.60 +41 39 26.6 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:51.60 +41:39:26.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 01.94 +43 18 08.2 14.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:01.94 +43:18:08.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 43.80 +41 23 12.3 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:43.80 +41:23:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 41.60 +41 01 11.6 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:41.60 +41:01:11.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 17.70 +41 05 12.1 14.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:17.70 +41:05:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 18.13 +42 02 14.0 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:18.13 +42:02:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 14.49 01:44:14.83 +49:40:51.5
131.63119 -12.29669 galactic And Second-epoch detections are separated by 4.0" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:44:14.83 +49:40:51.5 (user input) | T | P | (position from user input) SpType: A7V (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 14.83 +49 40 51.5 14.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:14.83 +49:40:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 33.13 +41 50 18.8 14.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347679771572574848,2461093.6803,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347679771572574848 20260222.1803 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:33.13 +41:50:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 35.59 +43 18 35.1 14.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:35.59 +43:18:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 56 41.72 +50 33 24.5 13.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0256419+503326,2461093.6803,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0256419+503326 20260222.1803 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:41.72 +50:33:24.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.47 01:46:00.02 +42:35:07.2
133.52422 -19.16142 galactic And Second-epoch detections are separated by 1.1" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347820646499640704 | 01:46:00.42 +42:35:13.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 00.02 +42 35 07.2 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347820646499640704,2461093.6803,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347820646499640704 20260222.1803 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:00.02 +42:35:07.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20_00sec_-15_00C_LIGHT_0257_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20_00sec_-15_00C_LIGHT_0257_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20_00sec_-15_00C_LIGHT_0257_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20_00sec_-15_00C_LIGHT_0257_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 23 03.21 +48 12 01.7 12.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0223030+481205,2461093.6803,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0223030+481205 20260222.1803 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:23:03.21 +48:12:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.92 01:42:11.71 +43:36:15.4
132.57736 -18.31482 galactic And Second-epoch detections are separated by 5.3" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348674039322200064 | 01:42:13.03 +43:36:16.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 42 11.71 +43 36 15.4 13.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348674039322200064,2461093.6803,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348674039322200064 20260222.1803 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:42:11.71 +43:36:15.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 36 24.20 +44 54 58.7 13.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:36:24.20 +44:54:58.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 48 15.68 +44 37 04.6 10.3 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J024815.79+443703.9,2461093.6803,10.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J024815.79+443703.9 20260222.1803 10.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:48:15.68 +44:37:04.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 18 55.22 +45 28 22.0 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J021855.32+452815.5,2461093.6803,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J021855.32+452815.5 20260222.1803 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:18:55.22 +45:28:22.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.62 01:46:16.24 +41:33:49.5
133.81850 -20.14598 galactic And Second-epoch detections are separated by 3.6" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347471688997166976 | 01:46:16.78 +41:33:56.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 46 16.24 +41 33 49.5 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347471688997166976,2461093.6803,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347471688997166976 20260222.1803 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:46:16.24 +41:33:49.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 59 56.11 +42 37 15.3 10.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IV Per,2461093.6803,10.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IV Per 20260222.1803 10.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:56.11 +42:37:15.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 28 25.37 +45 36 03.5 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.6803,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1803 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:28:25.37 +45:36:03.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.45 01:45:47.56 +44:49:48.8
132.96526 -16.98000 galactic And Second-epoch detections are separated by 2.9" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 350325260970638592 | 01:45:48.32 +44:49:50.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 45 47.56 +44 49 48.8 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 350325260970638592,2461093.6803,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 350325260970638592 20260222.1803 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:45:47.56 +44:49:48.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 11.92 01:40:54.69 +48:17:03.5
131.37083 -13.77513 galactic And Second-epoch detections are separated by 2.7" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 399335789917973632 | 01:40:54.45 +48:17:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.196+/-0.026 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 40 54.69 +48 17 03.5 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 399335789917973632,2461093.6803,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 399335789917973632 20260222.1803 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:54.69 +48:17:03.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 33 48.96 +45 12 54.0 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J023350.17+451256.9,2461093.6803,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J023350.17+451256.9 20260222.1803 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:33:48.96 +45:12:54.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.47 01:44:34.37 +40:54:48.1
133.64020 -20.85095 galactic And Second-epoch detections are separated by 4.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 347429495238424192 | 01:44:34.86 +40:54:53.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 44 34.37 +40 54 48.1 13.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 347429495238424192,2461093.6803,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 347429495238424192 20260222.1803 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:44:34.37 +40:54:48.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 32 11.23 +49 54 37.5 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0232117+495440,2461093.6803,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0232117+495440 20260222.1803 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:32:11.23 +49:54:37.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 02 33 46.26 +48 29 08.9 12.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J023347.4+482911,2461093.6803,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J023347.4+482911 20260222.1803 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:33:46.26 +48:29:08.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.41 01:43:52.46 +48:56:35.1
131.72728 -13.03112 galactic And Second-epoch detections are separated by 3.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J025.9710+48.9376 | 01:43:53.39 +48:56:32.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 43 52.46 +48 56 35.1 13.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J025.9710+48.9376,2461093.6803,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J025.9710+48.9376 20260222.1803 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:43:52.46 +48:56:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1803 2461093.6803 13.73 01:41:47.35 +42:23:36.6
132.76404 -19.51494 galactic And Second-epoch detections are separated by 1.6" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 348503374501213824 | 01:41:47.96 +42:23:46.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1803* 01 41 47.35 +42 23 36.6 13.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 348503374501213824,2461093.6803,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 348503374501213824 20260222.1803 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:41:47.35 +42:23:36.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20_00sec_-14_90C_LIGHT_0256_fits__*pix.png resample_wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.73814039 23.12.2025 05:42:45.330 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
First image: 2461032.73814039 23.12.2025 05:42:45.330 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
Last image: 2461093.68060128 22.02.2026 04:19:53.951 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 280
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 25651
Objects passed selection criteria: 25608
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 22748.2
Average stars matched: 22188.8 (97.5405 %)
Memory usage VmPeak: 128976 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Feb 21 22:31:08 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.73814039 23.12.2025 05:42:45.330 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
First image: 2461032.73814039 23.12.2025 05:42:45.330 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
Last image: 2461093.68060128 22.02.2026 04:19:53.951 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1920
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 204 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 167365
Objects passed selection criteria: 166988
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 145846
Average stars matched: 140522 (96.3496 %)
Memory usage VmPeak: 1988504 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Feb 21 22:38:34 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
And-03-Q2b1x1
#######################################
########### Starting And-03-Q2b1x1 ###########
Processing And-03-Q2b1x1
server tau has sufficient free disk space available: 1120049 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1120049 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.png' -> 'transient_report/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits_preview.png'
And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
renamed 'And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.png' -> 'transient_report/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits_preview.png'
And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 565.5119
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 778.3231
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1362.2390
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 753.1560
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1362.9513
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 752.6107
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.40886
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
No bad regions file found ../bad_region.lst
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
SExtractor catalog cache: saved And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat to cache
SExtractor catalog cache: saved And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461093.68004000
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits exists and is non-empty
Saving wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits to local_wcs_cache/
'wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits' -> 'local_wcs_cache/wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits'
wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits exists and is non-empty
Saving wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits to local_wcs_cache/
'wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits' -> 'local_wcs_cache/wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits'
wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
Saving wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits to local_wcs_cache/
'wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits' -> 'local_wcs_cache/wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits'
wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits exists and is non-empty
Saving wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits to local_wcs_cache/
'wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits' -> 'local_wcs_cache/wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:24:00.668 +45:59:40.33
Second-epoch image center 02:24:02.297 +46:00:24.11
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:24:00.668 +45:59:40.33
Second-epoch image center 02:24:01.341 +45:59:44.64
Angular distance between the image centers 0.00 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 02:24:02.297 +46:00:24.11
Second-epoch second image center 02:24:01.341 +45:59:44.64
Angular distance between the image centers 0.01131 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits &> /tmp/tmp.mi7XG7FrGI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits &> /tmp/tmp.XA4qutVhRZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits &> /tmp/tmp.1cegRRFbW7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits &> /tmp/tmp.8IwlpwoHYt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits and wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits and wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
Found non-empty wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits and wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
The reference image (wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits) and catalog (wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat) found
'wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 12290 out of 26534 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.939404
a=0.000000 b=1.000000 c=22.939404
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 234 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
2.1 pix And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
2.5 pix And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
2.5 pix And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Limiting magnitude estimates:
15.3 mag. And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
15.3 mag. And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
14.8 mag. And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
14.8 mag. And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mi7XG7FrGI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits' -> 'wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
WCS-calibrated image found: wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
Checking if the catalog wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
WCS catalog name: wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2580, passed=26534
Got 26534 stars (including 23926 good ones) from the SExtractor catalog wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 26534 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits -region wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.XA4qutVhRZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits' -> 'wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
WCS-calibrated image found: wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
Checking if the catalog wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
WCS catalog name: wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2625, passed=26432
Got 26432 stars (including 23774 good ones) from the SExtractor catalog wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat
util/solve_plate_with_UCAC5 got 26432 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 946 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits -region wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1cegRRFbW7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
WCS-calibrated image found: wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
Checking if the catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
WCS catalog name: wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2002, passed=19290
Got 19290 stars (including 17278 good ones) from the SExtractor catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 19290 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits -region wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8IwlpwoHYt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
WCS-calibrated image found: wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Checking if the catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
WCS catalog name: wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2023, passed=19227
Got 19227 stars (including 17197 good ones) from the SExtractor catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 19227 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits -region wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field And-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out30023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31710.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out31729.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out05353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31638.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31880.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 83s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 24s
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Considering the candidate 31582_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31582_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31589_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31589_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:00.32 +43:55:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.449 350180748209075840 025.75128376056 +43.93265473565 10.9866 10.5288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31591_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31591_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:36.34 +44:28:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.365 350258813534496896 025.40232740315 +44.47698754321 10.6034 9.9469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31592_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31592_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:45:10.09 +46:06:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.088 437141015473770752 041.29207691401 +46.10766532589 12.4289 12.1039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31593_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31593_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:30.56 +42:51:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.086 348613566182278912 025.62819882308 +42.85499322675 10.6337 9.9779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31595_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31595_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:08.76 +44:31:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 4.404 350224969192395008 026.03799290520 +44.53202008927 10.8267 10.2365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31596_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31596_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:56.59 +49:06:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 3.783 405388945026313600 025.73420743396 +49.11083570493 10.7030 10.1947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31597_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31597_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:21.29 +42:00:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 5.878 347730108589255808 026.08995847053 +42.00714828201 10.4865 9.8313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31600_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31600_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:24.53 +47:31:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.664 351238890711237760 025.60286680772 +47.52609824307 10.6214 10.0692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31602_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31602_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 31604_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31604_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:34.28 +47:39:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 5.038 351208993441448448 026.39491090879 +47.65501991566 10.6068 10.1122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31605_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31605_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:56.48 +49:48:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 3.292 405657668244128512 024.73401440104 +49.81050130247 10.1333 9.5000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31606_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31606_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31611_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31611_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:17.82 +48:32:56.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)
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Considering the candidate 31612_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31612_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:01.51 +46:24:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 3.426 351029605545249408 025.75491227324 +46.40691583831 10.5925 10.0323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31616_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31616_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:21.24 +46:30:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 1.683 351033900512508416 025.58799076868 +46.51177376509 10.3843 9.8971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31617_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31617_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 31618_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31618_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:55.43 +45:53:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 3.943 350637904528061696 025.22938504693 +45.88789450375 10.2766 9.7531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31619_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31619_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 31620_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31620_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:33.91 +47:09:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 1.200 351134849423650304 025.39150560635 +47.15764443963 10.2530 9.8185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31621_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31621_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 31625_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31625_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 31627_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31627_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 31628_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31628_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:43.93 +46:13:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 4.378 351020908233644416 025.68141330340 +46.22612440419 10.0672 9.5905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31630_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31630_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 31631_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31631_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 31632_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31632_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31636_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31636_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 31638_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31638_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31639_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31639_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 31640_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31640_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 31642_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31642_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 31643_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31643_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 31646_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31646_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:00.28 +49:06:14.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31647_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31647_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:19.32 +40:58:53.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31648_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31648_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:56.11 +49:16:49.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31649_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31649_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:48.50 +41:36:18.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31650_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31650_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:41.98 +48:54:17.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31652_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31652_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:51.38 +48:43:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.23, MAG_FAINT_SEARCH_LIMIT=11.21)GAIADR2_OUTPUT=# 3.575 405399562185693440 024.96558619500 +48.72161290761 9.2927 9.3100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31653_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31653_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:43.93 +41:18:42.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31654_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31654_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:59:56.08 +42:37:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)GAIADR2_OUTPUT=# 2.274 432427722659296256 044.98445068888 +42.62074281823 9.4103 8.1527 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31655_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31655_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31656_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31656_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31657_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31657_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31658_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31658_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31659_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31659_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:41.61 +50:53:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.49, MAG_FAINT_SEARCH_LIMIT=11.47)GAIADR2_OUTPUT=# 5.369 406203854941373312 025.67563999268 +50.89579362611 9.2007 8.7734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31660_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31660_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31661_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31661_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:46.94 +49:11:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 5.825 405614825946245760 024.69803295851 +49.18882160942 9.6836 9.3531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31662_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31662_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:09.86 +50:50:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.75, MAG_FAINT_SEARCH_LIMIT=11.73)GAIADR2_OUTPUT=# 4.029 405872661422629888 024.28962571586 +50.84519235271 9.1913 8.4399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31663_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31663_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31665_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31665_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31668_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31668_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31670_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31670_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:37.46 +48:28:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 3.839 399397706166292352 024.65769080681 +48.47195466586 10.0102 9.8936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31674_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31674_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31677_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31677_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31679_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31679_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31680_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31680_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:01.10 +48:48:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 3.513 405401451970977920 025.00586022061 +48.80449489525 9.9737 9.5232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31682_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31682_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31683_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31683_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31684_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31684_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31686_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31686_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31687_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31687_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31688_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31688_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31690_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31690_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:33.86 +50:02:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 5.582 405757590659295104 025.14347104815 +50.04846295965 10.5435 10.2985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31691_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31691_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 31694_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31694_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:23:28.95 +44:23:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.401 339980613196919424 035.87077931806 +44.38367908644 12.2037 11.7500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31695_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31695_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:11.25 +49:54:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 2.765 450706171463230592 038.04736214873 +49.91122884471 10.6931 9.1864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31696_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31696_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31698_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31698_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:27.48 +46:47:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 1.220 341974543174967552 039.36401060653 +46.79638377620 12.3323 11.8387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31701_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31701_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:43.88 +46:54:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 1.426 353798381981380992 036.18340554523 +46.90981391206 12.0528 11.3291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31702_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31702_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:19:03.26 +44:13:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.629 351902647839664000 034.76352007974 +44.23322434959 12.1627 11.6992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31703_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31703_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:19:55.38 +47:55:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.211 354839482055184768 034.98080890981 +47.92562676681 11.8673 11.1566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31704_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31704_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31706_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31706_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:27.80 +46:30:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.160 353719831322703232 037.11589163122 +46.51442532082 12.2092 11.8166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31707_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31707_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:34.98 +46:20:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.842 353710558490557056 036.89598863547 +46.34472141235 12.0374 11.3267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31708_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31708_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:42.80 +48:18:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 0.757 354338585788666880 037.17862491284 +48.30947042723 11.9156 11.1301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31709_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31709_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:13.14 +45:35:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.475 341423511752935680 038.30492952381 +45.59084896835 12.0568 11.3036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31710_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31710_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:56.83 +45:52:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.548 341631972286865024 037.73681359182 +45.87959594623 12.1413 11.6056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31711_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31711_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:49.34 +46:56:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.546 354118198129345280 036.95571590464 +46.94668387879 12.3130 12.0549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31712_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31712_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:45.12 +47:32:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.038 354162075516264704 037.43801557687 +47.53599809158 12.1783 11.6130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31713_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31713_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:25:52.13 +46:07:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.708 353693305606209792 036.46749099498 +46.13140726190 12.1652 11.5418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31715_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31715_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:38:11.26 +45:29:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.182 340996802459176704 039.54697564322 +45.48888781188 12.0701 11.3895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31716_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31716_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:17.16 +46:55:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.295 354115625446075392 037.07161780245 +46.91968389287 12.4783 11.9478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31717_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31717_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:00.43 +46:50:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.501 342104869661840384 038.00188280789 +46.84195789837 12.2543 11.7973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31718_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31718_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:57.61 +49:29:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.458 450494554130544256 038.49066445592 +49.48562783383 12.0222 11.2447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31719_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31719_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31721_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31721_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:38.53 +46:31:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.626 342082054795454592 037.41033517501 +46.52756622676 12.5162 12.0980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31722_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31722_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31723_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31723_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:22:08.40 +46:39:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.992 353865207377488512 035.53539171367 +46.65272682569 12.2242 11.6927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31724_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31724_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:31:57.23 +46:41:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.276 342099372103739264 037.98855546154 +46.68940641856 12.3082 11.8267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31725_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31725_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:34.46 +47:16:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.413 354176025570054784 036.89375046289 +47.26785025172 11.9654 11.0014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31726_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31726_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:39:09.26 +48:38:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.234 438468439543765888 039.78866779133 +48.64802219204 12.1910 11.7684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31727_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31727_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:17.03 +45:05:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.374 341480656295395712 037.32107566708 +45.09575719586 12.1203 11.4091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31728_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31728_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:12.95 +45:45:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.464 341659911049696512 036.80414303822 +45.75220049409 12.2520 11.7980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31729_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31729_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:27.06 +49:57:44.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)
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Considering the candidate 31730_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31730_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 31731_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31731_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:15.51 +45:31:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.084 341727634094573696 039.06501204729 +45.52584133381 11.5235 10.3636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31732_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31732_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:25:11.42 +46:46:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 1.275 353784599429516160 036.29803492677 +46.77747836228 12.3726 11.8935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31734_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31734_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:58.14 +48:42:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.240 354371536777835264 037.74234258548 +48.70794559011 12.1815 11.6472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31736_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31736_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:23:43.87 +43:33:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 1.392 339803694904320640 035.93237762274 +43.56136710052 12.7489 12.4172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31739_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31739_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:28.80 +45:23:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.302 341733818847260416 038.62006594015 +45.38437551219 12.2615 11.8260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31741_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31741_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:35:21.41 +46:15:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.346 341843078518150016 038.83933429732 +46.25665391022 12.3181 11.7714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31742_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31742_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:20:54.72 +46:54:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.423 353883967792906752 035.22856980095 +46.89998799452 12.7728 11.7106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31744_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31744_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:37.19 +46:30:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.165 341932310758696576 039.40501698795 +46.51256144249 12.2514 11.7419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31747_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31747_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:01.47 +47:42:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.637 354258592021386624 037.50600610375 +47.70396913176 12.9127 12.5521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31748_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31748_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:00.20 +45:32:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.431 341563699486613888 036.75139469100 +45.54080826801 12.4151 11.8505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31749_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31749_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31751_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31751_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:14:35.51 +47:02:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 1.264 354729664034037760 033.64846297655 +47.04934836274 12.3304 12.2241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31752_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31752_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:43.81 +48:21:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.432 354336867801734656 037.43272059780 +48.35312822063 12.2414 11.6584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31754_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31754_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:23:34.59 +48:43:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.414 354514640791440896 035.89429551856 +48.72396797048 12.0581 11.3574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31755_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31755_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:18.31 +48:31:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.120 450379650867147776 038.32633808129 +48.51742963921 12.2363 11.7539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31756_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31756_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:29.04 +46:14:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.251 341688253537062144 037.62097942719 +46.23512631404 12.1284 11.2254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31757_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31757_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:01.40 +46:01:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.657 353682207410807936 036.75585066169 +46.02012660817 12.4038 11.8742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31758_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31758_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:37.94 +44:51:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.456 341518275911362432 036.15805905959 +44.86279226764 12.2731 11.7681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31759_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31759_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:42.67 +46:44:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.198 342088754944384640 037.42786849757 +46.74648840503 12.3724 11.9792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31760_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31760_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:39:22.18 +45:43:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.480 341096819360536832 039.84242741627 +45.72546635508 12.3464 11.8993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31761_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31761_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:35:23.02 +47:17:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.756 342187229955394304 038.84622208005 +47.29470122802 12.0180 11.2291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31762_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31762_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:20:00.39 +45:25:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.813 352111387546940416 035.00188755395 +45.41874163249 12.2861 11.8907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31764_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31764_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:46.46 +47:22:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.500 354178469407160448 036.94416380192 +47.37174926846 12.9281 12.5279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31765_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31765_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:21.76 +47:47:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.745 354412527945406208 036.59096246439 +47.79719712578 12.1895 11.4242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31766_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31766_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:14.62 +47:14:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.304 354148778296481664 037.31102992535 +47.23765923188 12.3231 11.8783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31769_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31769_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:10.97 +46:15:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 0.873 353700143194143360 036.54605532621 +46.25145186366 12.4031 11.9388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31770_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31770_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:23:00.85 +46:31:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.602 353766010812590336 035.75378413013 +46.52632372875 12.4375 12.0546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31771_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31771_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:46.51 +45:44:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.289 341627402441667584 037.44388776367 +45.73454392633 12.3983 11.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31772_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31772_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:14.50 +46:52:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.661 353789169274716416 036.56056542765 +46.87193057253 12.2395 11.5055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31773_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31773_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:14.84 +46:52:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.389 342152079943239040 038.56196195058 +46.87897942661 12.3816 11.9104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31775_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31775_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:25:46.11 +45:49:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.634 353583290019805056 036.44230268027 +45.81915317199 12.3712 11.8540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31776_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31776_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:31:27.97 +46:09:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.395 342011716115194752 037.86667596383 +46.15096951302 12.2711 11.5634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31777_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31777_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:23:49.77 +45:07:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.884 353534499191458688 035.95745683894 +45.13243320197 12.3511 11.8775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31778_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31778_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:12.02 +45:03:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.783 341486012118395648 037.05038781522 +45.05522729830 12.3301 11.6505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31779_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31779_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:23:54.20 +47:23:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.332 354004707914149504 035.97596929186 +47.38991013511 12.1260 11.3857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31780_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31780_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:53.07 +48:04:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.506 438115393231444352 040.22133482034 +48.07965586844 12.3671 11.9515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31781_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31781_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:19:22.20 +47:47:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.281 354814708684003200 034.84261580039 +47.78818947348 12.1642 11.5079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31782_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31782_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:59.86 +44:45:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.124 340003870442787328 036.24936872975 +44.76108790124 12.1712 11.4178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31783_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31783_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:28.56 +45:05:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.476 341489722968811648 036.86918169775 +45.08691227635 12.1405 11.2013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31784_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31784_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:20:56.00 +46:17:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.740 353830229163833216 035.23361018460 +46.29438057449 12.3070 11.7914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31786_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31786_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:58.26 +47:35:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.511 342236261301646336 038.24259676921 +47.58868076738 12.2981 11.7317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31787_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31787_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:39:33.25 +46:20:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.100 341891358248736768 039.88855027620 +46.33677840995 12.3159 11.8876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31788_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31788_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:39.60 +46:14:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.132 353743917500824320 036.16505260757 +46.23521901179 12.3049 11.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31789_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31789_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:31:27.93 +45:47:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.432 341619160400164608 037.86652599333 +45.78777579637 12.2488 11.4606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31791_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31791_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:38.42 +45:44:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.501 341604694950102656 037.41027742595 +45.73997619186 12.2823 11.5854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31792_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31792_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:27.66 +45:51:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 5.612 353674132872204416 036.61741160432 +45.86179369910 12.6756 12.2078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31794_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31794_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:48.61 +45:49:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.216 341767388311751552 039.20262197489 +45.81758932468 12.3480 11.8091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31795_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31795_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:39:04.96 +47:30:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.991 438076424989993984 039.77107372167 +47.50095532376 12.2110 11.4905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31796_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31796_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:23.26 +47:58:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.470 342271475736118528 038.59701615673 +47.97627895276 12.4413 11.9941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31797_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31797_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:43.68 +45:44:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.560 341791813788529792 038.68217467109 +45.74284801472 12.2142 11.4235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31800_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31800_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:21:17.00 +45:15:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.767 352099980113962752 035.32113252301 +45.26308741634 12.2689 11.5213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31801_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31801_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:39:51.88 +46:47:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.796 341916715735253888 039.96647163858 +46.79146148041 12.3639 11.8500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31802_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31802_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:53.07 +48:24:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 1.028 354360610380936576 037.47152085743 +48.41422183119 12.2800 11.5660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31803_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31803_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:20:22.70 +44:02:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.747 351885639769209856 035.09481841860 +44.04248151740 12.1846 11.4639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31804_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31804_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:43.86 +47:35:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 1.788 354205059548959616 037.18348285289 +47.59647795301 12.4778 11.7888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31806_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31806_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:32.14 +47:07:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.531 342115143223548288 038.13493921644 +47.13078743939 12.3680 11.5704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31808_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31808_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:45:31.61 +46:25:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.916 437172214116193664 041.38191698413 +46.42901558801 12.2173 11.6617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31809_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31809_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:51.53 +47:11:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 2.359 354172761393864448 036.71518844242 +47.19120711703 12.5863 11.9266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31810_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31810_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:55.87 +46:27:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.249 341884310204196608 039.48278951663 +46.46134696608 12.3788 11.8583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31812_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31812_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:55.34 +45:23:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.263 353544497875286912 036.23067162679 +45.39278838204 12.4149 11.9035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31814_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31814_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:22.01 +45:57:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.191 341812979387349504 038.34178478139 +45.96527870971 12.4058 11.8550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31815_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31815_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:15.18 +45:12:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.448 341714474314865280 039.06342357662 +45.20677375794 12.3501 11.7302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31816_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31816_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:04.44 +47:46:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.666 354260000770657280 037.51866594222 +47.78328652966 12.1019 11.1792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31817_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31817_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:52.26 +46:51:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.327 342151869488381184 038.46788268466 +46.86375042875 12.3984 11.9514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31818_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31818_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:39.04 +47:44:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.381 438277021441164416 039.41279193490 +47.73645296471 12.4009 11.8370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31820_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31820_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:18:01.34 +47:33:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.550 354805053597487232 034.50580075520 +47.55231985414 12.2705 11.6554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31821_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31821_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:05.61 +44:25:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.712 339992669168095488 036.02338870504 +44.43166977195 12.3809 11.8534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31823_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31823_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:17:27.17 +46:29:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.924 353902900008731136 034.36357802393 +46.48414346580 12.2071 11.5281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31824_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31824_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:07.93 +45:18:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.602 340971067015010048 039.28324395649 +45.30689345379 12.5964 12.4254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31825_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31825_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:21:59.83 +48:03:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.724 354466438374602496 035.49938291341 +48.05605285764 12.0919 11.2325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31826_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31826_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:56.22 +44:12:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.249 341205774090938368 037.73434609619 +44.20771483075 12.2825 11.5854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31827_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31827_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:21:37.71 +47:58:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.443 354093360335745664 035.40726674230 +47.97641183029 11.9616 10.9661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31828_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31828_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:42:47.50 +47:25:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.429 438037186169860864 040.69808934936 +47.42733690903 12.4011 11.9967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31829_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31829_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:21:32.92 +48:13:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.261 355222077741623424 035.38723560628 +48.22933371753 12.1137 11.2968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31830_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31830_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:20:10.07 +44:54:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.229 352065169402109696 035.04197553568 +44.91467352829 12.3444 11.7682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31831_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31831_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:14.72 +46:47:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.627 342094248205617664 037.56158751240 +46.78993757979 12.4677 11.9589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31833_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31833_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:43:19.24 +46:21:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.598 437204447847091584 040.83012053776 +46.36052408979 12.2917 11.6159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31836_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31836_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:40.05 +47:45:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.157 354224545816164736 036.66732887496 +47.76451751539 12.4768 11.9542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31837_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31837_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:01.88 +45:32:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.514 341642245848385920 037.00798149761 +45.53751475127 12.4762 11.9762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31838_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31838_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:51.29 +48:57:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.291 450454245859169152 037.71380516862 +48.95753361074 12.3352 11.9130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31840_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31840_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:31:26.11 +46:15:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.239 342016767004230016 037.85874842960 +46.26228150375 12.9841 12.1879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31841_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31841_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:06.81 +48:07:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.256 354459497707655552 036.02848088203 +48.12296509028 12.4324 12.0536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31842_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31842_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:44:24.43 +47:36:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.681 438120031796529536 041.10197649724 +47.61047577780 12.1890 11.4449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31844_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31844_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:55.08 +47:09:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.546 342124008035852288 037.72968404515 +47.15580340788 12.5450 12.1419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31846_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31846_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:31:26.50 +47:34:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.272 354242958340431488 037.86052388100 +47.58227202368 12.4316 11.9316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31847_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31847_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:03.41 +45:45:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.605 341617304974291968 038.01444748272 +45.76554691124 12.6388 12.1618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31848_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31848_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:25:36.34 +46:22:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.285 353705748127039232 036.40144388494 +46.37932701314 12.6069 12.2886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31849_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31849_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:37.68 +46:28:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.372 341929630699098752 039.15707336789 +46.47995120797 12.2731 11.5410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31850_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31850_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:57:56.56 +47:45:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.202 437565190743045888 044.48615498888 +47.75972833156 11.0950 9.7906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31851_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31851_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:30.61 +44:11:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.138 339740262530023552 036.87755739265 +44.18992705820 12.5683 12.1226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31859_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31859_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:05.26 +47:46:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.164 354224099139554304 036.77224614609 +47.77045800663 12.4511 11.9971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31861_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31861_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:58.83 +44:16:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.569 339941782395582208 036.24523960989 +44.28194079474 12.4654 12.1572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31863_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31863_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:35.42 +46:20:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.447 342021096323764224 038.14776301193 +46.34592205293 12.2994 11.5851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31869_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31869_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:35:56.01 +45:06:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.516 341712270996051200 038.98348643722 +45.11592549929 12.4148 11.9575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31871_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31871_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:35.37 +43:56:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.465 339918731308387968 036.64747650721 +43.94832860381 12.2954 11.5960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31872_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31872_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:22:22.25 +47:21:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.298 354013267785782144 035.59280136925 +47.35322426192 12.5584 12.2480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31873_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31873_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:39:06.98 +46:51:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.452 341966365557182336 039.77924120334 +46.86174159794 12.4603 11.9193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31877_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31877_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:21.12 +48:32:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.363 438418033807883648 040.08813626171 +48.54418380480 12.4070 11.9695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31878_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31878_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:52.96 +48:28:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 0.840 438410745245030144 040.22100729101 +48.47405917368 12.0555 11.1283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31879_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31879_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:21:38.66 +45:37:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 0.760 353609192965477632 035.41133469850 +45.63278362112 12.4752 12.0621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31880_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 31880_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 31881_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31881_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:25:33.38 +47:10:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.780 353809029203513600 036.38930852215 +47.17909781479 12.4968 12.0216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31884_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31884_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:51:48.87 +45:40:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.124 433982294662028416 042.95366446957 +45.67393729443 12.1080 11.4352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31885_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31885_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:44.01 +45:59:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.150 341833767029061376 038.68336069646 +45.98484590290 12.4947 12.0454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31887_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31887_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:30.80 +47:28:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.526 342239937793666688 038.62854898407 +47.47201929306 12.4956 12.0061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31889_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31889_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:38.11 +48:18:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.371 450365494654945792 038.40888609829 +48.30863732736 12.3352 11.6634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31894_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31894_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:57:00.91 +49:28:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.303 439411511283911424 044.25512463201 +49.47744186171 10.9132 9.4903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31899_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31899_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:44.05 +48:25:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 0.758 354349714046458496 037.68362689447 +48.43164730662 12.5083 12.0453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31901_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31901_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:35:10.43 +45:06:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.564 341340636064484992 038.79362989810 +45.11237701845 12.5226 12.2622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31902_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31902_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:50.81 +47:58:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.030 354324356560613248 037.21170020591 +47.98067302411 12.5356 12.2343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31907_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31907_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:19.49 +44:12:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 1.016 340526069747359104 039.08104083835 +44.20233877412 12.4866 12.1940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31908_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31908_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:14:25.15 +45:57:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.796 353113042640510080 033.60505927486 +45.95553610038 12.3410 11.8688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31911_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31911_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:18.01 +46:43:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.680 341952965259018240 039.07500991100 +46.73249325088 12.6207 12.2779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31912_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31912_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:38:21.78 +47:52:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.352 438273649889141376 039.59078431071 +47.87423402257 12.6247 12.4360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31913_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31913_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:38:00.84 +48:01:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.552 438310693984576768 039.50351875050 +48.03245830528 12.5608 12.0491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31916_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31916_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:25:16.53 +47:56:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.553 354406476334237952 036.31909520578 +47.94609813590 12.2353 11.4004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31918_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31918_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:45:37.00 +46:53:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.455 437247225721177344 041.40427448339 +46.89574144305 12.4226 11.9434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31919_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31919_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:44.74 +47:07:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.765 342208734854433792 038.18647262847 +47.13168116293 12.5380 11.8186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31920_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31920_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:21:00.74 +43:50:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.744 339868905391376128 035.25331616595 +43.83753729460 12.3304 11.7063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31922_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31922_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:15:47.73 +47:13:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.905 354692589876357504 033.94924197468 +47.23185471486 12.3785 11.8485 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31925_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31925_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:23.79 +49:19:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.490 354644417524173312 036.59925608235 +49.32543915394 12.2240 11.4635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31926_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31926_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:32.55 +49:53:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.497 450602679931493120 038.63626457571 +49.88758436616 12.4771 11.9530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31927_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31927_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:20.18 +48:09:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.533 354329544881098112 037.08428641826 +48.15822664844 12.2505 11.4625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31936_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31936_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:30.90 +46:41:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.774 353772337299743232 036.12902025092 +46.69305343657 12.4384 11.7945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31937_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31937_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:35:54.43 +46:24:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.228 341939599320901248 038.97687100644 +46.40953188810 12.4744 11.8214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31938_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31938_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:35:55.40 +46:46:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.646 341953991753597312 038.98108639398 +46.77804624387 12.3214 11.4934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31940_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31940_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:35:16.65 +48:46:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.326 450401370520792448 038.81930238631 +48.77804906455 12.5257 12.0397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31942_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31942_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:42:02.40 +46:48:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.158 437983967232080000 040.51004544180 +46.80280890960 12.3626 11.7005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31946_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31946_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:37.47 +48:06:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.579 438115629451444608 040.15635930582 +48.11410190992 12.3902 11.8569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31951_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31951_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:42.98 +48:30:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 0.152 438383089953057792 039.17914551614 +48.51415745298 12.5134 12.1076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31955_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31955_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:30.07 +43:39:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.010 339667905218218880 037.37548238295 +43.66096658750 12.3935 11.8578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31980_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 31980_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:20:28.93 +44:00:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.264 351882616112234240 035.12094248918 +44.01200582920 12.6072 12.2461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06744_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 06744_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08118_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 08118_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06295_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 06295_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05353_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 05353_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12882_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 12882_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 30023_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 30023_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:25.57 +47:28:30.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 111s
Prepared the HTML report for the field And-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:35:51.44 +49:18:00.8
02:52:22.70 +48:39:52.3
02:11:02.76 +48:56:44.2
02:32:53.71 +48:20:16.8
02:32:46.05 +46:29:20.8
01:45:57.46 +49:08:31.1
01:42:50.83 +43:56:33.5
01:42:04.22 +48:01:55.3
01:37:53.07 +50:36:24.1
01:39:31.97 +50:29:42.3
01:44:36.44 +41:10:50.4
01:39:19.25 +49:36:17.6
01:40:52.67 +50:18:02.5
01:38:04.85 +49:25:59.4
01:38:22.85 +49:17:20.3
01:45:30.58 +49:51:02.0
01:39:41.54 +49:00:13.9
01:40:40.90 +50:16:46.3
01:40:24.74 +49:45:59.4
01:40:39.39 +45:07:34.2
01:39:55.75 +46:38:07.0
01:40:43.59 +50:37:31.8
01:41:14.46 +46:52:03.6
01:39:50.16 +50:35:55.4
01:44:21.07 +50:27:44.5
01:37:49.92 +50:22:14.3
01:44:15.38 +42:56:25.3
01:45:27.42 +50:12:18.1
02:25:53.93 +46:25:30.0
01:40:36.95 +50:47:45.7
01:40:05.55 +50:08:11.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
SExtractor catalog cache: saved And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat to cache
SExtractor catalog cache: saved And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
Creating symlink local_wcs_cache/wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
Creating symlink local_wcs_cache/wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
Creating symlink local_wcs_cache/wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits exists and is non-empty
wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits exists and is non-empty
wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:24:00.668 +45:59:40.33
Second-epoch image center 02:24:02.297 +46:00:24.11
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:24:00.668 +45:59:40.33
Second-epoch image center 02:24:01.341 +45:59:44.64
Angular distance between the image centers 0.00 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 02:24:02.297 +46:00:24.11
Second-epoch second image center 02:24:01.341 +45:59:44.64
Angular distance between the image centers 0.01131 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits &> /tmp/tmp.qJ1t8OXJ0x
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits &> /tmp/tmp.vE8aTSyUFf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits &> /tmp/tmp.V33eHn6uIa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits &> /tmp/tmp.0mr9TK0Gd6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits and wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits and wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
Found non-empty wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits and wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
The reference image (wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits) and catalog (wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat) found
'wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 12467 out of 177487 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.802346
a=0.000000 b=1.000000 c=22.802346
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.51
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1406 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
1.9 pix And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
2.4 pix And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
2.4 pix And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Limiting magnitude estimates:
15.5 mag. And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
15.5 mag. And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
15.0 mag. And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
15.0 mag. And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.qJ1t8OXJ0x (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits' -> 'wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
WCS-calibrated image found: wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
Checking if the catalog wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits
WCS catalog name: wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=22518, passed=177453
Got 177453 stars (including 154660 good ones) from the SExtractor catalog wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 177453 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 947 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits -region wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-03-Q2b1x1_2025-12-22_23-42-45_20.00sec_-14.90C_LIGHT_0256.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.vE8aTSyUFf (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits' -> 'wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
WCS-calibrated image found: wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
Checking if the catalog wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits
WCS catalog name: wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=22738, passed=178849
Got 178849 stars (including 155836 good ones) from the SExtractor catalog wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat
util/solve_plate_with_UCAC5 got 178849 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 946 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits -region wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-03-Q2b1x1_2025-12-22_23-43-36_20.00sec_-15.00C_LIGHT_0257.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.V33eHn6uIa (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
WCS-calibrated image found: wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
Checking if the catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits
WCS catalog name: wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=16009, passed=115943
Got 115943 stars (including 99819 good ones) from the SExtractor catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 115943 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits -region wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-05_20.00sec_-14.90C_LIGHT_0099.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0mr9TK0Gd6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
WCS-calibrated image found: wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
Checking if the catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat corresponding to the image wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits
WCS catalog name: wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=15802, passed=115279
Got 115279 stars (including 99367 good ones) from the SExtractor catalog wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 115279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010421 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-03-Q2b1x1_222034_TTUQ2b1x1_17998_0QNuVVPB/And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits -region wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field And-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out157991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203097.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203125.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203714.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203905.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204141.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204419.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204553.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204663.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205194.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out205728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out97229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out203355.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203541.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203574.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203665.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203717.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out203823.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204218.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204429.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out204903.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out03551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out105213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out159879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203358.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203445.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203672.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203692.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203722.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204277.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204296.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204304.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204335.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204363.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204767.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205077.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205164.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205216.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205392.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24530.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out40721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58280.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 762s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 287s
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Considering the candidate 202810_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 202810_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 202812_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202812_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 202813_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202813_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:02.24 +42:04:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 3.171 347592669635708160 027.25820685075 +42.06880622184 13.3676 12.8932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202818_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202818_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:03.05 +46:38:58.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)
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Considering the candidate 202826_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202826_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:58.58 +46:32:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.985 353722309521060096 036.99482607471 +46.53909831185 14.6345 14.1264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202828_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202828_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:38.85 +42:30:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.539 347851570264042752 025.91279429474 +42.51197277288 13.0718 12.4730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202841_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202841_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:46.69 +44:40:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.558 350322585209038976 026.44394899713 +44.67281864528 13.0938 12.4311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202842_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202842_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 202847_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202847_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:30.51 +43:16:14.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)
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Considering the candidate 202849_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 202849_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 202851_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202851_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:11.45 +45:46:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 3.911 350624469870606976 025.79861602645 +45.76904932642 13.3264 12.8898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202853_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202853_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:02.25 +46:57:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.671 437997573688093312 040.00992828674 +46.95881352890 14.7532 14.1994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202854_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202854_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:22.99 +45:32:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 5.787 350743973040094336 026.59807948935 +45.53715408352 13.0813 12.5633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202855_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202855_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:17.86 +41:49:32.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)
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Considering the candidate 202856_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202856_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 202859_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202859_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:37.47 +46:16:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.108 350845334268122112 026.40696171610 +46.27185289858 12.8968 12.2425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 202860_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202860_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:25.26 +43:32:20.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)
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Considering the candidate 202862_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202862_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:39.15 +44:39:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 4.544 350320145667621504 026.16391197724 +44.65154789076 13.2382 12.9200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202863_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202863_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:39.67 +44:38:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 4.792 350286954160176256 025.66347087248 +44.63838903867 13.1572 12.4858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202870_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202870_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 202871_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202871_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:32.57 +46:59:15.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)
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Considering the candidate 202872_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202872_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:51:52.79 +42:54:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 2.072 349144183621567488 027.96947863440 +42.90804418177 13.1869 12.4548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202875_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202875_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:23.95 +47:47:43.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)
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Considering the candidate 202877_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202877_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:41.67 +42:06:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.705 347604863045743488 027.17272160058 +42.10418787244 13.1579 12.5644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.705#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202880_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202880_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:10.24 +42:22:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.659 340050191668116224 039.29315736771 +42.37636803904 14.7659 14.2634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202881_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202881_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:33.24 +42:12:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 3.589 347739037823404800 026.13835502791 +42.20906431371 12.5778 11.9755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202882_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202882_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:58.95 +43:42:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.985 349462183000709376 027.74635880516 +43.70965057122 13.4050 12.7853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202883_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202883_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:06.18 +44:56:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 4.347 350379347496982528 026.02738269788 +44.93826131575 12.8618 12.3445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202885_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202885_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:52.83 +50:27:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.758 357988964393459072 027.21953068072 +50.46291608775 12.9343 12.1964 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202887_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202887_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:58.60 +41:25:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.340 347492648437259392 027.74418909276 +41.42145536455 13.0710 12.3398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202888_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202888_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:12.94 +41:52:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 0.538 347564185412339840 027.30407169987 +41.86973829621 13.0066 12.3147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202889_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202889_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:24.02 +42:06:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.277 347605314019002880 027.09929867142 +42.11255803358 12.9690 12.4905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202890_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202890_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:39.55 +40:59:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.183 347424822314168448 026.41592915378 +40.99484368279 12.5625 11.8114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202891_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202891_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:40.36 +41:36:28.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)
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Considering the candidate 202897_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202897_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:17.20 +43:11:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.252 349339690533340672 027.07119438970 +43.19942235590 13.1851 12.6640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202902_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202902_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:18.15 +42:59:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.536 349324881486013184 027.07686728693 +42.98648399605 13.1227 12.6101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202903_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202903_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:43.27 +43:25:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 3.927 348655863020237184 025.93142756408 +43.41775881262 12.8279 12.1953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202904_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202904_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:49.26 +41:11:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.257 344486240049608320 027.70565782160 +41.18599961284 12.9172 12.4251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202907_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202907_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:09.65 +43:35:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.785 349418168175506816 026.78983595608 +43.59561160392 12.9903 12.2358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202911_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202911_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 202915_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202915_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:02.54 +46:10:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 4.317 350843955581033984 026.51149698212 +46.18207422260 13.1097 12.6562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202919_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202919_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:52:17.31 +50:30:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 1.680 357954153680547712 028.07158693734 +50.50867841573 13.0243 12.5482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202920_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202920_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:54.66 +40:57:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 5.087 347429907555280512 026.22913357664 +40.96445155512 12.8483 12.3616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202925_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202925_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:54:23.93 +50:12:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 4.822 357931686709909120 028.60052170137 +50.21592851303 13.2600 12.7710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202928_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 202928_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 202929_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202929_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:55.05 +47:28:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.472 357193227212253696 026.72892987515 +47.46766062797 13.0193 12.4561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.472#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202932_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202932_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:22.88 +46:38:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 3.547 399132071029439104 024.84665433367 +46.64092087023 12.5908 11.9282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202933_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202933_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:51.22 +41:56:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.372 347568411660144256 027.21299207381 +41.94945334572 13.0161 12.6065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202935_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202935_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:08.22 +49:47:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 4.829 405888363824398592 026.53583252243 +49.79899152476 12.6849 12.1578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202936_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202936_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:00.45 +43:42:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 2.800 350173906323127552 025.75207097411 +43.70940188902 12.7943 12.3481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202937_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202937_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:10.35 +48:33:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 4.328 357320976719067776 026.04493302211 +48.55289256777 12.8882 12.3529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202939_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202939_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:10.06 +44:01:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.478 340672721407059968 040.04248437756 +44.03176242933 14.3861 13.6564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202940_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202940_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:08.23 +48:51:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 0.936 357422681545023232 026.53426187370 +48.85550934878 12.9002 12.3322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202941_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202941_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:56:44.73 +41:01:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.348 336128646007996800 044.18686816680 +41.03273504469 13.7832 13.0280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202942_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202942_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:51.85 +44:32:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 0.760 340549129427466240 038.71608753977 +44.53984754773 14.5105 13.9180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202944_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202944_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 202945_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202945_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:13.81 +41:01:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.130 347387645077423744 027.30771193352 +41.02749130879 12.7781 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202946_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 202946_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 202947_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202947_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:05.74 +50:17:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 1.796 405927460908640000 026.77368312171 +50.29910736468 12.8701 12.3636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202948_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202948_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:46.15 +41:09:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 4.440 347406439854093056 026.94123267540 +41.16553121415 12.6384 12.0203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202949_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202949_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:26.40 +47:41:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.669 351253802837623808 025.85975632018 +47.68445033481 13.0081 12.4385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202951_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 202951_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 202954_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202954_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 202958_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202958_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:57.49 +50:00:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.975 357873442656559488 027.48923212802 +50.00598870536 13.2079 12.6235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202959_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202959_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:51:19.20 +49:05:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 4.050 357757379757346432 027.83047367488 +49.09544249831 13.2574 12.7699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202961_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 202961_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 202962_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202962_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:10.91 +48:39:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.481 357313726814399616 026.54568143297 +48.65700481020 12.8553 12.3374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202965_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202965_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:55.13 +44:20:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.693 350253895794422656 025.47935894033 +44.33554601712 12.7627 12.2691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202966_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202966_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:17.46 +43:41:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.260 348674829595543296 025.57265787680 +43.68675032217 12.6881 12.1275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202968_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202968_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:49.35 +47:34:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.337 357021909556473600 027.45658611247 +47.57294215571 13.1287 12.5988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202969_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202969_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:43.34 +43:25:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.209 348655863020237184 025.93142756408 +43.41775881262 12.8279 12.1953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202971_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202971_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 202974_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202974_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:42.89 +47:24:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 2.470 351236962270439040 025.67924646773 +47.40838694133 12.7181 12.1847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202976_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202976_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:48.77 +44:26:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 5.619 349551926339191040 026.95444489691 +44.43592603186 13.2620 12.5924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202977_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202977_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:55.02 +43:49:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 4.129 348724857374585728 025.48038644304 +43.82030184630 12.7484 12.0052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202979_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 202979_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 202980_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202980_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:35.23 +43:28:08.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)
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Considering the candidate 202981_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202981_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:51.41 +42:18:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 3.329 347743852484551808 025.96532180616 +42.30883744870 12.5086 11.8491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202982_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202982_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:05.02 +42:05:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.602 347768866374035072 026.52133861295 +42.08710035631 13.1260 12.5973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202983_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202983_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:53:17.58 +47:42:43.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)
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Considering the candidate 202987_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202987_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 202988_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 202988_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 202990_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202990_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:06.65 +46:44:27.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)
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Considering the candidate 202991_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202991_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:34.66 +46:18:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 2.311 351035515420411008 026.14368754134 +46.30329668178 12.7958 12.1228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202993_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202993_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:29.52 +44:41:17.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)
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Considering the candidate 202996_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 202996_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 202998_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202998_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:51:22.47 +50:47:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 3.401 358009133559709440 027.84253089608 +50.79313410922 12.6922 11.8767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202999_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 202999_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:27.35 +44:31:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 3.760 350270942522125440 025.86528056383 +44.52011592807 12.7324 12.0518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203002_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203002_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:53:25.95 +51:01:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 3.243 359516357843534848 028.35896498976 +51.02507585876 12.8471 12.2614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203005_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203005_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:58.45 +48:41:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 3.145 357363578497913856 026.99224876380 +48.68345233244 12.6121 12.1460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203006_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203006_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:22.85 +43:04:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 5.855 349381197097184768 026.59329763560 +43.06755702416 13.1157 12.5924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203007_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203007_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:22.68 +45:51:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.038 350824752784925184 026.59518846950 +45.86668995048 12.9900 12.4803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203008_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203008_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:16.34 +48:25:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.732 405342971696342784 025.31813551114 +48.42753543039 12.6829 12.1742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203009_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203009_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:50.75 +44:09:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.959 349530004826122368 026.96196932065 +44.15081872507 13.1469 12.6386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203011_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203011_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:25.31 +49:08:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.797 357397839454308992 027.35478297471 +49.13721237986 12.9139 12.4714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203012_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203012_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:28.71 +44:18:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.025 350217749349661824 026.11990214431 +44.30476803610 12.7939 12.3698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203014_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203014_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:15.85 +49:44:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 4.824 405512674444464640 026.56802202643 +49.73456356830 12.7025 12.1825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203015_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203015_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:03.37 +48:08:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 2.132 357285620546251776 025.76349442015 +48.14988300404 12.8481 12.2093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203016_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203016_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:02.23 +41:29:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.870 336947438573415808 040.00929449845 +41.48560283511 14.2063 13.5868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203017_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203017_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:02.80 +41:27:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.423 347460487722476544 026.76185951749 +41.45965736253 12.7554 12.2218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203018_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203018_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:53:01.97 +41:06:14.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 203019_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203019_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:53.61 +40:51:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.643 347238695610684672 025.72348146453 +40.85199278333 12.2123 11.5374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203020_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203020_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:44:46.69 +41:39:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 0.570 336859374563632128 041.19453438942 +41.65682503660 14.2839 13.8486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203023_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203023_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203028_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203028_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:08.05 +44:43:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 3.801 350291347909221888 025.53440363068 +44.72897331838 12.5731 11.8871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203030_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203030_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:57:26.08 +51:02:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 0.642 359299646675276544 029.35888069042 +51.04885499272 13.0185 12.5423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203032_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203032_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:22.50 +49:17:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 0.975 405479135041825536 026.09413750417 +49.29820823382 12.4468 11.9649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203034_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203034_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:12.02 +49:35:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 4.059 405542361258207616 025.55182124492 +49.59489732366 12.5824 12.0687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203035_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203035_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:46.99 +45:55:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.715 351001769859380608 025.94540946309 +45.92770097063 12.5313 12.2209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203037_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203037_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:37.85 +46:43:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.662 351098118863249536 025.15706129641 +46.73195462481 12.5833 12.0641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203039_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203039_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:08:24.96 +48:10:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.284 435949320968638464 047.10452128112 +48.18138542340 13.9437 13.2821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203041_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203041_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:54:14.14 +50:55:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.734 359465367991822208 028.55732381570 +50.93273938804 12.5687 12.0997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203043_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203043_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:23.86 +44:19:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 3.067 350262691887446144 025.84834242590 +44.32247875892 12.8567 12.4214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203045_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203045_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:21.42 +45:04:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.690 350498399693251968 025.08982397305 +45.07093118556 12.4649 11.7877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203046_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203046_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 203047_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203047_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:30.90 +44:02:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 4.060 350229229799888128 025.63025773702 +44.04724293565 12.6775 12.1509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203048_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203048_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203050_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203050_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 203052_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203052_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203056_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203056_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:25.80 +44:03:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.613 350194148507153280 026.35745329055 +44.06521996231 12.7354 12.0421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203057_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203057_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203058_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203058_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:02.54 +42:16:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.861 347786355480652032 026.26065683646 +42.28001075826 12.7703 12.3490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203060_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203060_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:53:48.65 +49:24:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.020 357606055171087104 028.45285733709 +49.40896081429 13.0589 12.5674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203061_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203061_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:15.34 +48:49:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 4.629 357386015407112704 027.31527517484 +48.82331276333 12.9146 12.2943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203063_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203063_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:05.42 +46:29:01.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)
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Considering the candidate 203067_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203067_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 203070_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203070_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:56:53.75 +51:01:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.401 359481169173058560 029.22404598500 +51.02147423112 13.0230 12.2949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203071_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203071_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 203074_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203074_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 203076_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203076_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:28.26 +46:02:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 3.586 350830211685692288 026.61645672438 +46.03962362837 12.5938 12.0307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203079_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203079_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 203080_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203080_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:08:56.11 +47:21:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 0.676 435770753405412224 047.23377691313 +47.36504856441 13.6671 13.0514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.676#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203082_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203082_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203084_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203084_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:49.50 +42:44:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 3.192 347825456862968448 026.70743241176 +42.73918161242 12.7508 12.2571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203085_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203085_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:33.23 +50:27:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.908 405942377332848768 026.63857851637 +50.45611433896 12.3821 11.8979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203086_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203086_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:08.63 +48:23:05.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)
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Considering the candidate 203087_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203087_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 203089_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203089_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 203090_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203090_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:41.15 +46:55:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 5.544 351162332917595776 025.92367601522 +46.91844405508 12.7718 12.3318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203091_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203091_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:01.31 +44:31:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.077 350279665598185984 025.50587478512 +44.51932443526 12.5901 12.1307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203092_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203092_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:12.59 +43:16:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 0.306 339643922121183104 037.55234534721 +43.27257710105 14.3624 13.7144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203094_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203094_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:21.87 +41:10:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.759 344481257887548544 027.59071725992 +41.17852970446 12.7571 12.2188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.759#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203097_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203097_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:18.68 +46:37:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 1.507 351049529895689216 026.07810930465 +46.62173427564 12.7209 12.3078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203098_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203098_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:05.12 +44:48:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.967 350327361212639360 026.27202089856 +44.81453140639 12.7526 12.2919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203100_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203100_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:26.23 +43:16:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 1.267 349398819345053696 026.35918736214 +43.27257308380 12.5484 12.1194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203101_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203101_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:30.06 +44:14:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.655 350246821985878784 025.37470410470 +44.23761855747 12.5507 12.0726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203102_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203102_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:48.98 +47:01:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.220 351131787110729216 025.45492685157 +47.02291607759 12.5438 12.0807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203103_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203103_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:11.61 +47:13:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 0.838 351214731518595328 025.79858637261 +47.22540021473 12.4318 11.8850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203104_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203104_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203105_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203105_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 203107_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203107_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:55.92 +46:42:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.556 351098526883973888 025.23335219113 +46.70261000017 12.5248 11.9670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203109_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203109_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:51:53.29 +49:03:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.313 357569530769192960 027.97154625617 +49.05027822125 12.8868 12.1712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203112_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203112_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:34.70 +44:37:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.536 350322099874721536 026.39359370496 +44.62675889194 12.8355 12.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203113_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203113_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:52:37.04 +41:30:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.316 344517438691972096 028.15506184487 +41.50197991998 13.0929 12.5265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203115_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203115_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:05:22.37 +42:56:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 3.245 240364340027866624 046.34443942740 +42.94704619706 13.8756 13.4434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203116_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203116_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 203117_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203117_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:44.88 +47:07:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.251 351130898053743360 025.18609524577 +47.11922407225 12.5475 12.0680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203118_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203118_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:20.80 +49:57:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.154 357855747391301504 027.08635993036 +49.96324063046 12.6148 12.1452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203120_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203120_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:52.38 +44:21:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.244 350216134441954944 025.96797339330 +44.36135565360 12.5956 11.9897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203121_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203121_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:46.43 +44:16:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 0.158 349548597742414208 026.94349143101 +44.28110188332 12.8699 12.3280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203122_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203122_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:52.52 +47:02:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.840 351153158867448320 026.46951752181 +47.03704068515 12.7524 12.3175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203123_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203123_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 203124_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203124_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:50:19.19 +49:53:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 1.497 438787778952586752 042.58051343928 +49.89976766297 14.1529 13.4866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203125_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203125_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:27.69 +49:05:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 3.244 357431920017555968 026.61400672264 +49.09426351706 12.6583 12.1067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203126_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203126_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:54.12 +43:27:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.435 340409010415293184 038.47525088509 +43.46007738229 14.6626 14.1521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203127_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203127_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:34.46 +48:15:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.646 357298780328314368 026.39330285705 +48.25124925336 12.8131 12.3154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203129_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203129_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 203130_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203130_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:49.97 +49:04:35.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 203131_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203131_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:54:11.48 +50:29:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.897 357945464964903424 028.54798588495 +50.49681527428 12.9613 12.4338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203132_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203132_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 203133_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203133_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:08.91 +42:25:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.721 347616274775611520 027.28699529939 +42.41983710793 12.8668 12.3600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203134_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203134_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:53.08 +44:04:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.943 350197034725176064 026.22156619434 +44.07131830963 12.7668 12.3478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203135_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203135_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:55:56.84 +50:54:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.640 359456464521175296 028.98812459083 +50.90153934781 12.8774 12.3169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203138_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203138_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:56:07.42 +51:04:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.173 359483922250706560 029.03121111659 +51.08299113533 12.8032 12.3063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203139_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203139_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 203140_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203140_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:31.96 +45:13:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.294 349974108742011776 027.38149659158 +45.23010794534 13.0114 12.4603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203141_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203141_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:02.97 +45:59:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 4.919 350818185777265152 026.26431116497 +45.98737877337 12.7614 12.2599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203143_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203143_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:01.63 +50:16:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.034 405925055726956160 027.00705519430 +50.27481612277 12.3997 11.6861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203147_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203147_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 203148_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203148_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:30.43 +48:50:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.397 357411098016119936 026.62734917380 +48.83942908602 12.5321 12.0446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203149_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203149_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203150_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203150_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203152_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203152_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203155_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203155_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 203157_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203157_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:18.63 +41:43:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 3.922 347666439994240768 026.57695479533 +41.71742108565 12.4555 11.8358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203159_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203159_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203163_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203163_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:53.98 +48:59:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.775 357426873432868480 026.22406083048 +48.99019485218 12.5519 11.8012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203165_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203165_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:12.03 +45:22:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.025 350597527538857728 025.29898705383 +45.36906461837 12.3910 11.6421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203166_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203166_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203167_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203167_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:11.42 +45:06:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.855 350382401215598976 026.04830033585 +45.11123646731 12.5895 11.9226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203169_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203169_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:50.25 +47:30:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.185 399274109892470400 025.20930411315 +47.50410205484 12.3272 11.8480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203171_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203171_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:01.31 +44:43:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.339 350312552165421952 026.50668351126 +44.72648652324 12.7804 12.2526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203172_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203172_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 203173_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203173_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:22.51 +43:34:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.501 349412052141947904 026.34453007130 +43.58319323465 12.9056 12.3973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203174_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203174_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:03.66 +42:37:47.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 203175_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203175_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:57.46 +48:48:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.237 357385774888945280 027.23969574609 +48.81395464313 12.7635 12.2266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203181_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203181_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203182_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203182_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:29.22 +43:10:39.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
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Considering the candidate 203184_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203184_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 203187_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203187_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:15.96 +47:55:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 3.387 357267650405226496 026.06790247009 +47.92901094374 12.6322 12.1008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203188_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203188_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:51:55.49 +49:43:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 5.048 357804624397517312 027.97918880950 +49.72206727909 12.6510 12.1172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203190_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203190_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 203192_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203192_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203193_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203193_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:16.84 +46:54:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.217 351104406695337728 025.06926872714 +46.90391921471 12.5003 11.8876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203195_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203195_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:06.36 +43:05:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.722 348622843311568512 025.77815958492 +43.09236247248 12.5226 12.0743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203196_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203196_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:53:10.91 +50:55:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.827 359514154523632768 028.29581858764 +50.93146598082 12.5975 12.1106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203197_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203197_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 203198_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203198_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:51:00.04 +49:49:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 4.978 357820739114793984 027.74830703085 +49.83260457512 12.7720 12.2712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203199_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203199_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 203200_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203200_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:12.94 +44:48:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.190 350336707061474304 026.55399714169 +44.80990895271 12.6584 12.1953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203201_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203201_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 203202_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203202_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:32.13 +44:50:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.795 350336256086915712 026.63280802639 +44.83656283001 12.6234 12.1644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203203_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203203_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:06.22 +49:46:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.775 357852693671153792 027.02554865171 +49.78354303544 12.5340 11.9056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203204_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203204_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 203205_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203205_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:38.24 +46:08:57.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 203206_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203206_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:59.79 +41:12:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.563 344486583646983936 027.74857016631 +41.21589779760 12.4647 12.0457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203207_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203207_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:25.68 +41:50:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.802 347704544943940736 025.85752474325 +41.83327138266 12.2161 11.6743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203208_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203208_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:22.90 +47:53:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 4.258 351273761548765824 025.84697569847 +47.89299793598 12.5669 12.0591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203210_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203210_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:26.57 +48:32:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 5.372 357320044709228928 026.10846310461 +48.53764907864 12.2807 11.7983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203211_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203211_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203212_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203212_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203215_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203215_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:17.32 +41:47:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.845 347562703646782976 027.32380017152 +41.78540595171 12.6072 12.2012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203216_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203216_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:42.59 +46:42:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.817 351062625253711616 025.92744844057 +46.70446742576 12.7062 12.2073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203217_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203217_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:53.88 +44:24:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.436 350302205586215936 026.47401529566 +44.41494647822 12.6929 12.2286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203218_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203218_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203219_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203219_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203221_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203221_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 203223_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203223_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:54.67 +49:23:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.261 357825510820041344 027.22683768719 +49.38860109068 12.7228 12.1960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203225_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203225_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203232_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203232_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 203233_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203233_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:07.82 +49:03:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.361 357420065907820800 026.78033077636 +49.06405977112 12.1324 11.4443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203234_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203234_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:34.95 +44:43:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 3.671 350321137802043008 026.14699375035 +44.71958441786 12.5039 11.8814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203235_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203235_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203238_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203238_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203239_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203239_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 203241_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203241_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:52:49.50 +49:38:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.209 357799741016279808 028.20660448966 +49.64458833775 12.8563 12.2383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203244_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203244_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:04:46.88 +42:05:55.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)
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Considering the candidate 203245_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203245_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203247_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203247_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:29.56 +45:40:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 4.172 350807087582451712 026.12481923677 +45.67945640918 12.4643 11.7980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203249_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203249_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:42.83 +49:02:50.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)
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Considering the candidate 203250_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203250_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:46.36 +44:45:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.843 350368008782959104 025.94424218754 +44.75572872702 12.3263 11.6116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203252_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203252_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:23.75 +48:53:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.303 357411579052453120 026.59831777258 +48.89426812698 12.5218 12.0645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203253_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203253_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:00.05 +43:45:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.932 350163323523708032 025.99990145802 +43.75777291056 12.3378 11.6591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203254_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203254_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:52:24.67 +48:57:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.796 437918958608520832 043.10299958556 +48.96481311863 14.2346 13.5375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203256_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203256_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:01.42 +44:18:19.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 203258_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203258_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:10.59 +45:46:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.533 350621029598512512 025.54507681902 +45.77359765375 12.6368 12.0583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203260_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203260_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:37.11 +46:07:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.231 350872031785054720 027.40455450654 +46.11941158433 12.8562 12.3915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203261_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203261_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203262_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203262_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203263_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203263_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:33.04 +49:11:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.635 405471992514181120 026.13616487932 +49.19780556187 12.3537 11.8291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203264_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203264_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:25.51 +44:42:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.757 350286090869252480 025.35557008982 +44.70387576008 12.3158 11.8765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203265_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203265_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:00.91 +48:02:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 2.829 357226143841476992 026.50262068562 +48.03709475635 12.6990 12.1447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203266_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203266_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:53.72 +44:00:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 4.454 350185111895974912 025.97523688881 +44.01738204382 12.4980 11.8659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203268_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203268_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 203270_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203270_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203271_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203271_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:01.62 +47:52:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.185 399289331254532736 025.25460787800 +47.87307112933 12.2231 11.7214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203272_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203272_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:58.04 +47:02:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.804 351120177815384704 025.49143873864 +47.03958922254 12.2916 11.9025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203274_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203274_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:08.16 +48:12:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 5.074 399323381754765440 025.53212421295 +48.21170693033 12.3628 11.8120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203275_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203275_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:26.49 +48:00:01.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 203276_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203276_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:32.54 +48:18:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.114 357302315084893440 026.38640148076 +48.31597102309 12.3766 11.8316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203277_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203277_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:18.11 +49:03:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.619 357384847175993472 027.57697463414 +49.06198613825 12.7790 12.3361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203278_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203278_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203279_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203279_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:54:37.82 +49:51:34.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 203280_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203280_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203283_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203283_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:38.92 +42:59:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.224 347881703754477440 026.41209997377 +42.99292192057 12.6150 12.0139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203286_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203286_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:24.86 +47:45:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.604 357215080005822208 026.35211717540 +47.75531385873 12.5180 11.9581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203287_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203287_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:18.32 +47:35:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.969 351249572292462720 026.07558892916 +47.59116174539 12.4741 11.8837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203288_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203288_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203289_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203289_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 203290_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203290_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 203291_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203291_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:19.72 +42:33:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 4.088 347854800079285248 025.83068720975 +42.54984802367 12.1784 11.5235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203292_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203292_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203293_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203293_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203295_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203295_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:52.75 +45:41:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.040 350622472708915072 025.71951872753 +45.68836689487 12.4994 12.0089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203296_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203296_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 203297_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203297_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 203298_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203298_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:05.92 +46:08:34.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 203299_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203299_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:18.82 +50:29:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.302 405971273872519680 026.07840943953 +50.49261047867 12.3513 11.8592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203300_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203300_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:04.37 +43:32:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.298 349452905871375872 027.51897075749 +43.53785279572 12.7394 12.0200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203301_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203301_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:52:18.53 +50:51:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.586 358011946760538624 028.07679476023 +50.85767285219 12.4495 12.0193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203302_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203302_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203303_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203303_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 203304_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203304_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 203307_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203307_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:02.63 +44:30:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.055 350224453796323456 026.00944155150 +44.50063034603 12.3573 11.6763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203308_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203308_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:36.52 +49:04:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.415 405390486916869760 025.65101648876 +49.07949332373 12.3780 11.8390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203309_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203309_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:56:30.77 +50:49:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.558 359267417240697344 029.12752377714 +50.82120927699 12.6237 12.1511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203311_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203311_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:08.86 +47:29:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.209 399195013772240896 024.78602567062 +47.48868674543 12.0435 11.2518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203313_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203313_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 203314_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203314_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:15:47.68 +44:19:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.475 352126265314192768 033.94860941281 +44.32876953537 14.2296 13.9625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203315_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203315_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:58.74 +49:14:47.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 203316_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203316_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203318_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203318_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:32.73 +41:04:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.644 347423551003826304 026.63616200813 +41.07621756168 12.1983 11.5363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203319_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203319_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:51.61 +50:14:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.513 405924510268996992 026.96621929678 +50.23329651393 12.3462 11.8420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203322_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203322_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203323_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203323_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 203326_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203326_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:58.54 +41:00:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 4.446 344478229932806272 027.49301076680 +41.00441585722 12.4930 11.7296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203328_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203328_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:05.37 +47:47:11.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)
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Considering the candidate 203330_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203330_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:04.78 +45:22:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.712 350421777475749504 026.01968676127 +45.38208046347 12.5982 12.0318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203334_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203334_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:30.27 +50:52:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.724 406182856845083392 025.37550107585 +50.87682834693 12.0320 11.2706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203335_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203335_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:39.96 +45:51:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.308 350810115536386560 026.16750166924 +45.85957026369 12.3099 11.5827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203337_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203337_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 203338_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203338_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:45.38 +47:50:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.136 399297165275280384 024.93744038862 +47.84974013405 12.2054 11.5226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203339_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203339_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203342_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203342_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:11.80 +45:07:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.461 350347255501250176 026.79990051835 +45.12664077937 12.7881 12.1795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203343_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203343_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:44.81 +48:20:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.724 405327475454572544 025.68610951811 +48.34534979080 12.2399 11.7334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203347_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203347_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:47.61 +45:41:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 5.543 350611722407490176 025.19656349128 +45.69615502755 12.3768 11.8645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203348_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203348_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:47.08 +41:08:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.949 347392318001826944 027.19524103126 +41.14776406397 12.3309 11.8235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203351_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203351_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:49.64 +47:18:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.180 351197379850717696 026.20827292006 +47.30809349769 12.3788 11.8462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203354_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203354_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:10.70 +47:12:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.350 351228200537160064 025.54588773786 +47.20932677692 12.4308 11.9540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203355_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203355_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:55:54.60 +48:29:35.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
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Considering the candidate 203356_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203356_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:20.46 +45:27:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.885 350426484759902080 025.83338453350 +45.45888712940 12.3745 11.9374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203357_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203357_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 203358_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203358_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203361_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203361_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:36.73 +49:34:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.643 357470712161658496 026.65454959193 +49.56804508897 12.3383 11.8516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203362_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203362_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:04:37.77 +50:27:04.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)
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Considering the candidate 203363_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203363_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 203364_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203364_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:38.99 +47:52:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 4.322 351274242585103616 025.91354212094 +47.87676665354 12.3723 11.7376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203366_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203366_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:55.54 +49:59:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.992 357878596617314944 027.23152868760 +50.00066220203 12.3663 11.8519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203368_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203368_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:52.61 +49:52:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.483 405563900517103872 025.46865310463 +49.86760158788 12.0104 11.3473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203370_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203370_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:24.38 +49:35:28.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
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Considering the candidate 203372_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203372_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 203373_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203373_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 203374_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203374_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:14.09 +48:26:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.976 357342722136735360 027.30942256446 +48.43663938779 12.5750 12.1151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203376_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203376_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:42.07 +43:55:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.279 350180537753042560 025.67521293494 +43.91925280780 12.2244 11.7874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203377_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203377_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 203378_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203378_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:51:03.42 +48:27:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.720 357175699448828672 027.76466429195 +48.46316871461 12.6984 12.0932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203379_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203379_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203380_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203380_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 203381_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203381_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:45.22 +49:20:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.106 357449993239928320 027.18795372458 +49.33527523476 12.2784 11.5573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203382_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203382_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:20.77 +45:40:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 0.557 341764673892480128 039.08640183662 +45.68270319992 14.5859 14.2502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203386_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203386_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:01.46 +46:37:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.031 350954220278863872 026.50594143709 +46.63082485559 12.3562 11.7886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203387_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203387_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:11.48 +46:49:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.724 351122853578735488 025.29714587563 +46.82809028532 12.3764 11.8576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203388_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203388_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 203390_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203390_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 203391_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203391_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 203393_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203393_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 203394_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203394_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 203395_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203395_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203396_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203396_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:41.70 +48:35:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.288 405359563152303488 025.92361101058 +48.59178787890 12.1612 11.4987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203397_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203397_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:53.41 +45:34:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.471 350432600793328384 025.97198573212 +45.56954196524 12.2100 11.7386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203398_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203398_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:52:38.77 +51:00:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 4.559 359518483850663680 028.16352189995 +51.01541107577 12.4581 11.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203399_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203399_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:35.56 +43:24:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.111 349401121447515264 026.39788692698 +43.40043444353 12.3443 11.6850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203400_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203400_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203401_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203401_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:22.47 +42:22:11.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 203402_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203402_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 203403_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203403_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:10.83 +47:33:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.533 351249125615864320 026.04574439074 +47.56435932082 12.3655 11.8824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203405_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203405_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:28.39 +50:00:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.950 405905470675496320 026.37010991040 +50.00627533904 12.1270 11.4789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203406_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203406_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:36.56 +45:38:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 5.581 350806129806787968 026.15421469366 +45.63701484199 12.3888 11.8718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203409_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203409_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:49:40.87 +40:57:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.131 335995639460589184 042.42069268690 +40.95366658614 13.7728 13.2021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203410_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203410_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 203411_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203411_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:48.09 +46:39:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.808 351059837817198336 025.69985838940 +46.65508376006 12.1368 11.5690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203412_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203412_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 203414_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203414_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 203415_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203415_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:38.59 +48:19:59.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)
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Considering the candidate 203416_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203416_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:01:04.83 +43:09:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.651 432561485121395840 045.27104813579 +43.16570172466 13.6852 13.1543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203418_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203418_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:53.96 +42:53:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.523 347831160579510656 026.72576344402 +42.89244184528 12.3933 11.8725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203419_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203419_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203420_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203420_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 203421_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203421_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:07.39 +44:41:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.405 350366840552057088 026.03289355551 +44.68763241746 12.2458 11.7269 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203422_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203422_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:46.04 +47:20:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.148 351187381166023552 026.69099412302 +47.34118080082 12.3195 11.8280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203423_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203423_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:21.75 +43:38:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.674 349433694479476352 026.59053892995 +43.63596069286 12.2696 11.7128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203424_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203424_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:38.54 +45:03:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.642 350486721679138304 025.15902553987 +45.04943918252 11.9802 11.3408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203425_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203425_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:44.39 +50:11:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.128 357891039138963584 027.18405323749 +50.19281184325 12.0969 11.7155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203426_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203426_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:51:40.62 +48:06:03.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
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Considering the candidate 203427_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203427_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:54.82 +45:43:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 5.058 350808290173290368 026.23035208872 +45.72946862450 12.4797 11.9341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203428_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203428_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:07.40 +48:36:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.851 405340051118752640 025.78061779812 +48.61266552131 12.2538 11.7740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203429_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203429_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203430_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203430_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:10.93 +45:22:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 3.576 350421609974849536 026.04683461784 +45.38131892553 12.2875 11.7973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203431_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203431_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:54.22 +49:00:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.885 357438487024858112 026.97531511794 +49.00532265143 12.8241 12.3314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203432_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203432_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:44.87 +42:28:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.845 347796418586510080 026.43629234944 +42.47954845335 12.3447 11.8377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203436_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203436_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:05.24 +41:39:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.862 347476258842356352 026.77241734075 +41.65208331978 12.3814 11.8721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203439_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203439_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203442_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203442_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:00.24 +41:10:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.365 347392760381077632 027.25255506485 +41.17856694858 12.3670 11.7151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203443_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203443_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 203444_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203444_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:47.55 +41:55:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.998 347582052476148096 026.94894216777 +41.93348500803 12.3086 11.8431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203445_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203445_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203446_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203446_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 203447_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203447_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203448_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203448_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 203450_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203450_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203453_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203453_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:55:26.14 +41:06:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.070 345933609668796288 028.85936931282 +41.10493522024 12.6758 11.9951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203454_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203454_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 203455_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203455_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 203457_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203457_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:01.57 +47:55:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.333 357229098779200128 027.00791523093 +47.93123856919 12.4226 11.9042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203458_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203458_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203459_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203459_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:55.80 +45:54:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.701 350816128490588672 026.23211133394 +45.91069974483 12.3992 12.0071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203460_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203460_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:56:31.77 +50:45:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.360 359266626966718592 029.13304170404 +50.76433524144 12.6036 12.0913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203462_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203462_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 203464_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203464_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 203465_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203465_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:45.47 +45:22:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.781 350598287749878656 025.18744348523 +45.37874092199 12.0861 11.4245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203466_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203466_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:16:29.83 +49:33:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.656 355535472915912704 034.12484979811 +49.55213494641 13.6938 12.9027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203467_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203467_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 203469_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203469_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 203470_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203470_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:23.10 +43:01:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 5.829 347892076099566336 026.09756071632 +43.02544488623 12.1068 11.5756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203471_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203471_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 203473_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203473_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 203474_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203474_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 203476_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203476_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203477_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203477_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:04.66 +42:07:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.878 347782163592775424 026.51917308505 +42.13225262858 12.2204 11.7864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203478_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203478_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203480_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203480_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:41.50 +48:36:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.181 357322140653267328 026.17262884303 +48.61526053799 12.2549 11.7987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203481_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203481_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 203482_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203482_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:24.71 +45:48:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.130 350800872766776320 026.60376429034 +45.80230880165 12.2533 11.6037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.130#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203484_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203484_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:10.82 +43:55:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 4.370 349482038632039296 027.29676017687 +43.92476680066 12.4042 11.9106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203485_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203485_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.6") between the two second-epoch detections
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Considering the candidate 203486_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203486_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 203487_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203487_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:46:19.77 +42:32:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.452 337296911472306816 041.58283378969 +42.54605351223 13.8918 13.2037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203488_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203488_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 203489_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203489_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 203490_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203490_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:36.27 +47:22:14.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 203491_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203491_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203495_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203495_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 203496_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203496_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 203498_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203498_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:09.20 +46:45:20.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 203500_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203500_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203502_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203502_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 203503_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203503_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 203504_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203504_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:11.78 +50:42:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.836 405954742540937344 026.54930485344 +50.71448161797 12.0129 11.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203509_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203509_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:37.29 +44:12:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.142 350213316943420800 025.90605741562 +44.20174482146 12.0637 11.5533 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203513_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203513_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203514_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203514_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:03.77 +44:28:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.787 350224415138893952 026.01420682868 +44.47762881725 12.2083 11.5405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203515_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203515_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:32.05 +50:18:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.383 405939830414451840 026.63414175343 +50.31349749133 12.1194 11.6439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203519_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203519_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 203521_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203521_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:24.44 +47:56:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.224 357229644238264576 027.10162972317 +47.93760524171 12.4284 11.9344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203523_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203523_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:06.16 +47:09:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.621 351169479743166464 026.27459866088 +47.16117175206 12.3276 11.8479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203524_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203524_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:47.41 +45:41:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.592 350630719046123264 025.44602489625 +45.68693219056 12.1052 11.6763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203525_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203525_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:58.22 +49:47:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 5.865 405525353187625600 025.99010420497 +49.79180435848 11.9776 11.4387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203527_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203527_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203529_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203529_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203531_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203531_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:50.84 +48:24:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.366 357315341721997440 026.21131580238 +48.41207775838 12.0964 11.7779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203532_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203532_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:06.09 +45:35:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.603 350617941520368640 025.52557276876 +45.58670546894 12.0691 11.6249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203533_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203533_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:01.32 +43:16:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.584 348648230860411648 025.75518257231 +43.26818004739 11.9935 11.4214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203535_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203535_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:14.46 +48:04:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.053 357284379300812416 025.81064221783 +48.08375637090 12.1189 11.6317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203537_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203537_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203538_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203538_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 203540_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203540_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:27.93 +44:34:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.386 350283548248618880 025.36517624447 +44.56657793755 12.0514 11.5708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203541_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203541_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:10.82 +46:03:29.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)
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Considering the candidate 203542_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203542_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 203543_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203543_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 203544_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203544_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203547_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203547_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 203548_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203548_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 203550_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203550_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 203552_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203552_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 203553_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203553_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:42.63 +48:28:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 5.333 357296714446878336 025.92980548733 +48.46710009587 12.0560 11.5479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203554_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203554_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:46.57 +43:01:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.682 347891461920170240 025.94275765152 +43.02971091333 11.9338 11.2707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203555_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203555_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:55.96 +42:31:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.362 347620187488387456 027.23365697905 +42.52305436322 12.2234 11.7654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203558_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203558_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:31.58 +49:48:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.363 405572456091961216 025.88100716863 +49.81171012049 11.9233 11.3590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203560_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203560_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:00.58 +46:06:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.939 351007507935683840 025.75124905747 +46.10992148823 12.0772 11.5351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203561_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203561_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203562_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203562_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 203566_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203566_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 203567_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203567_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:55:50.63 +50:28:00.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 203568_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203568_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:09.20 +46:38:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.426 350953601803570816 026.53968168091 +46.64630470343 12.3292 11.8400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203571_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203571_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 203574_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203574_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:51.51 +45:30:02.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 203576_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203576_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 203579_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203579_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:42.67 +41:42:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.035 347514741748854656 027.42698080524 +41.70871896154 12.0636 11.4251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203580_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203580_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 203581_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203581_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:53:59.23 +50:41:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.564 357960239652337408 028.49664252913 +50.69892401333 12.0960 11.6089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203582_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203582_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 203583_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203583_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:41.55 +49:02:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 5.562 357392788572812032 027.17548172341 +49.03640798709 12.1098 11.5836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203585_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203585_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:00.47 +45:17:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.975 350411336413097728 026.25174546320 +45.28877769940 12.0738 11.6231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203586_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203586_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 203589_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203589_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 203590_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203590_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 203592_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203592_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:55.20 +44:56:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.148 350379484935553664 025.98036199828 +44.94564159703 11.9016 11.3028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203593_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203593_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 203594_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203594_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203595_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203595_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:51.17 +46:26:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.863 351040974320843392 025.96211662314 +46.43961892953 12.0295 11.5785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203597_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203597_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 203598_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203598_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 203599_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203599_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 203601_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203601_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:35.36 +50:10:38.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 203602_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203602_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:27.75 +49:48:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.928 405516793315805696 026.36470110604 +49.80939893758 12.0182 11.4707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203603_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203603_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 203604_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203604_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 203605_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203605_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:52.44 +48:13:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.637 354428814461216512 036.71913677988 +48.23110814888 13.3146 12.5162 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203606_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203606_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:15.98 +45:17:15.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 203612_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203612_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 203614_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203614_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203617_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203617_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:03.41 +45:58:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.679 351002182176240000 026.01456457259 +45.96822950348 11.9465 11.5104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203618_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203618_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 203620_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203620_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:33.75 +44:03:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.503 349449225082857856 026.64029645817 +44.06312214978 12.0122 11.5750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203621_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203621_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:29.38 +48:22:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.996 357302766057931520 026.37354263353 +48.36861491773 11.9771 11.5317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203622_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203622_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:34.14 +44:33:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.987 350269018376769664 025.64123981940 +44.55480978678 11.9572 11.4899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203623_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203623_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 203624_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203624_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:33.03 +45:31:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.510 350605812532739200 025.38817507900 +45.52877701444 11.7183 11.0433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203625_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203625_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 203626_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203626_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 203627_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203627_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203628_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203628_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:33.27 +45:02:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.384 350357352966333952 026.63652579127 +45.04438610548 11.8637 11.3438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203629_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203629_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:31:47.96 +47:34:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.448 354240179498543360 037.95041797623 +47.57007797566 13.5072 12.8047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203630_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203630_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203632_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203632_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203633_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203633_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 203634_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203634_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 203635_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203635_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 203637_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203637_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:10.12 +46:48:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.047 351146836675572608 026.29053046601 +46.81359550707 11.8793 11.5139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203638_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203638_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:33.88 +46:12:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.198 351013520889896064 025.89112935171 +46.20202062761 11.7796 11.3605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203639_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203639_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:00.46 +43:44:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.695 349427101707437952 027.00088404884 +43.74545176875 12.0188 11.4899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203640_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203640_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:12.46 +44:31:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 3.659 350314201432910592 026.30332997829 +44.52097832531 11.6741 11.0276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203642_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203642_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:16:32.29 +47:27:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.971 354718741933889536 034.13469601216 +47.45255434832 13.5778 13.0823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203646_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203646_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:37.39 +45:31:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.023 350789907713282816 026.40548900646 +45.51777265294 11.8593 11.3081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203647_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203647_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:10.07 +44:46:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.167 350327047677037184 026.29040558749 +44.77856280836 11.8501 11.4165 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203649_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203649_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 203650_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203650_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 203651_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203651_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 203653_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203653_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 203655_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203655_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203656_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203656_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:51:37.19 +41:53:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 5.669 347531921618159616 027.90697699541 +41.89294322222 11.8255 11.2892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203658_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203658_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:52:23.77 +50:52:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.631 358013462887038080 028.09883935438 +50.87762900748 11.7307 11.2827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203661_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203661_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 203662_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203662_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 203663_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203663_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 203664_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203664_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:45.09 +47:08:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.337 351180131262061312 026.43653387574 +47.14094274315 11.7884 11.3856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203665_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203665_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:12.95 +48:08:51.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)
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Considering the candidate 203669_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203669_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 203670_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203670_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 203671_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203671_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:53.43 +44:42:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.934 350332064198844544 026.72455117919 +44.70311829676 11.8384 11.3603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203672_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203672_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203674_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203674_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:58.34 +43:37:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.920 350163705779028352 026.24234904277 +43.62681814209 11.8413 11.5197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203675_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203675_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 203676_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203676_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 203677_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203677_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 203678_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203678_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 203679_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203679_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 203680_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203680_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 203682_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203682_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:33.93 +47:28:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.365 351226589924918272 025.89315043671 +47.46766166125 11.6512 11.1980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203683_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203683_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203684_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203684_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 203685_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203685_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 203687_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203687_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203688_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203688_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 203692_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203692_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203693_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203693_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:31.32 +49:29:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.396 405503294235935360 026.38260707471 +49.49591609921 11.4755 10.9429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203695_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203695_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:12.42 +44:26:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.266 350299559886360960 026.55376752002 +44.44017046581 11.7180 11.2126 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203699_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203699_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203700_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203700_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:54:30.15 +50:25:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.750 440281946537152640 043.62612321758 +50.42211826912 12.6155 11.7250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203701_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203701_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:43.85 +43:32:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.176 349418370036167936 026.93200777631 +43.54971686525 11.7463 11.2360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203705_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203705_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 203706_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203706_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203710_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203710_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203714_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203714_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:08.06 +49:19:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.852 357775830936668160 027.53575737730 +49.32046323915 11.6345 11.0858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203715_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203715_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:05.44 +47:53:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 4.195 357208753518642432 026.77094910385 +47.89215006608 11.7215 11.2038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203716_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203716_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 203717_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203717_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:33.89 +42:35:57.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)
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Considering the candidate 203718_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203718_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 203719_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203719_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:51:33.76 +40:59:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.668 344469025820730624 027.89008464310 +40.99841403762 11.4917 10.8560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203720_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203720_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 203721_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203721_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203722_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203722_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203723_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203723_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:48:09.52 +48:21:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 0.737 437796290045207552 042.03996639409 +48.36186902743 13.0352 12.5517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203724_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203724_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 203726_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203726_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 203728_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203728_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:07.52 +50:21:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 0.914 405929183193356800 026.78115576480 +50.36310617242 11.3687 10.8560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203729_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203729_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 203730_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203730_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 203731_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203731_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203732_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203732_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 203733_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203733_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 203734_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203734_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 203737_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203737_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:10.64 +43:37:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 4.606 350161472396035712 026.04258834022 +43.62621354724 11.2230 10.6189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203739_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203739_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:05.36 +47:24:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 1.714 357192844957456256 026.77167713401 +47.41013388474 11.4521 11.0148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203740_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203740_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 203741_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203741_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203743_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203743_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203744_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203744_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 203745_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203745_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:01.64 +44:45:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 4.614 350326845816576768 026.25862189160 +44.76228441478 11.3012 10.6535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203748_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203748_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 203749_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203749_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:18.51 +44:06:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.649 350189166344933376 025.82836344430 +44.10709776090 11.1642 10.5403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203750_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203750_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 203751_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203751_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 203752_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203752_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 203753_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203753_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 203754_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203754_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 203755_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203755_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 203756_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203756_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 203758_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203758_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 203759_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203759_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:22.36 +48:40:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.039 357349701461066752 027.34189753513 +48.68032332499 11.3066 10.8077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203760_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203760_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 203761_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203761_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 203762_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203762_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:28.37 +46:32:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 3.387 350949886655417088 026.61689255728 +46.54472926801 11.2716 10.7128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203763_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203763_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 203764_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203764_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:52:04.67 +50:22:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 3.710 357929728204980480 028.01793481566 +50.37595441369 11.1572 10.6442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203765_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203765_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 203766_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203766_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 203767_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203767_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 203768_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203768_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203769_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203769_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 203770_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203770_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 203771_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203771_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203773_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203773_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 203774_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203774_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:59.97 +47:56:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.897 357044930581068032 027.50022423829 +47.93741417256 11.1759 10.6281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203777_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203777_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 203778_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203778_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 203779_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203779_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 203780_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203780_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203781_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203781_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:27.66 +48:10:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.793 357145364096329216 027.36491995391 +48.18243675436 11.0187 10.4787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203783_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203783_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 203784_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203784_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 203786_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203786_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 203787_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203787_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 203788_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203788_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:02.02 +44:27:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.614 350313582957629056 026.25754118170 +44.46332427794 10.8220 10.1552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203789_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203789_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 203791_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203791_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 203792_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203792_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 203794_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203794_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203796_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203796_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203797_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203797_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:06:18.11 +48:17:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.072 436147473579845376 046.57547748990 +48.29629325162 11.9486 11.6290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203799_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203799_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:31.98 +49:08:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 2.494 357446973880173568 027.13219154350 +49.14943942605 10.7499 10.3222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203800_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203800_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:27.72 +48:39:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 4.060 357358222675894784 026.86385766637 +48.65197419577 10.6810 10.1779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203801_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203801_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 203802_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203802_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 203803_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203803_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:59.66 +48:23:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 1.337 357295511856036992 025.99810246002 +48.39943994466 10.4275 10.0563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203804_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203804_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 203805_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203805_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 203806_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203806_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:31.13 +46:43:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 5.220 351142576068016128 026.37762146588 +46.72790434677 10.5582 10.0716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203807_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203807_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 203808_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203808_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 203809_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203809_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:20.08 +46:25:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.467 351031942007453696 025.58267870083 +46.42447865200 10.2588 9.8712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203810_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203810_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 203811_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203811_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 203813_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203813_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 203814_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203814_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 203815_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203815_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203816_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203816_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:56.88 +46:19:53.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.31, MAG_FAINT_SEARCH_LIMIT=12.29)
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Considering the candidate 203819_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203819_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203822_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203822_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 203823_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203823_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:36.70 +42:17:38.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)
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Considering the candidate 203824_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203824_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 203825_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203825_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 203826_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203826_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:58.42 +43:52:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.27, MAG_FAINT_SEARCH_LIMIT=11.25)GAIADR2_OUTPUT=# 5.649 350191434087855232 026.24554595580 +43.88179961836 8.8881 8.2567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203827_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203827_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 203831_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203831_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:52.31 +49:39:25.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 203832_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203832_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:36.42 +48:24:58.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 203833_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203833_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:59.97 +49:06:12.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 203834_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203834_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:28.79 +48:15:12.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 203836_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203836_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 203837_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203837_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:26.08 +40:58:26.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 203838_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203838_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:25.92 +42:11:04.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 203839_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203839_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:41.93 +48:54:17.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 203840_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203840_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 203841_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203841_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203844_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203844_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:51.30 +48:43:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.61, MAG_FAINT_SEARCH_LIMIT=11.59)GAIADR2_OUTPUT=# 4.379 405399562185693440 024.96558619500 +48.72161290761 9.2927 9.3100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203845_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203845_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:36.38 +41:10:48.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203846_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203846_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203849_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203849_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:38.45 +48:48:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 2.474 405404338188996736 025.16125029842 +48.81587579312 9.4161 9.2934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203850_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203850_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203851_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203851_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:58.38 +48:12:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 2.195 399331490653494144 024.99233945374 +48.20300356412 9.2307 8.7887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203852_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203852_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:19.40 +49:36:16.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203853_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203853_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203854_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203854_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:53.69 +50:36:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.85, MAG_FAINT_SEARCH_LIMIT=11.83)GAIADR2_OUTPUT=# 4.956 405856271827519488 024.47583759355 +50.60587545795 9.1428 8.9692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203855_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203855_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 203856_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203856_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:32.60 +50:29:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 5.556 405802666339748096 024.88815413353 +50.49393960485 9.2939 9.1990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203857_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203857_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203859_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203859_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:15.54 +48:02:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 2.062 399352179513247872 024.81552629455 +48.04615882934 9.4433 9.0890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203861_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203861_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:22.27 +46:49:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 3.704 399135610082471808 024.84428193861 +46.82833434675 9.7147 9.4556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203867_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203867_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:23.61 +49:10:16.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)
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Considering the candidate 203868_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203868_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 203871_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203871_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:08.06 +42:37:55.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)
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Considering the candidate 203874_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203874_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:30.42 +49:51:02.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203875_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203875_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:46.97 +49:11:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 5.470 405614825946245760 024.69803295851 +49.18882160942 9.6836 9.3531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203877_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203877_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:32.46 +48:22:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 1.491 399340016165766784 025.13565892930 +48.37814599621 9.9297 9.6885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203879_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203879_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:01.23 +47:49:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 4.590 399296409360638464 024.75659792061 +47.82383266070 9.9592 9.5780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203881_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203881_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:09.86 +50:50:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 4.029 405872661422629888 024.28962571586 +50.84519235271 9.1913 8.4399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203882_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203882_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:51.80 +49:47:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 2.571 405668427137872896 024.46665652047 +49.79972707885 9.4603 8.8079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203884_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203884_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:04.75 +49:25:58.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203885_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203885_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:22.74 +49:17:19.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203886_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203886_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:15.48 +50:17:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 2.609 405778275221561216 024.56361980534 +50.28509600262 9.4643 8.7600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203891_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203891_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:41.87 +49:00:13.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203899_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203899_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:37.38 +48:28:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 4.635 399397706166292352 024.65769080681 +48.47195466586 10.0102 9.8936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203902_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203902_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203903_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203903_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 203905_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203905_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:57.00 +49:25:15.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)
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Considering the candidate 203906_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203906_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:39.54 +45:07:35.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203912_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203912_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:55.55 +46:38:07.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203913_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203913_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203914_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203914_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203916_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203916_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 203917_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203917_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:05:46.69 +43:43:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 1.532 432916455578880768 046.44453051472 +43.72003655472 11.3785 11.0390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203918_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203918_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203921_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203921_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:36.05 +45:21:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.575 350596810281131904 025.15197635315 +45.36257346114 10.1652 9.7976 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203923_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203923_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:41.75 +42:51:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 5.857 347872151747245568 026.42559076273 +42.86396368860 10.1070 9.5216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203925_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203925_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203926_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203926_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203928_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203928_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203929_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203929_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:18.35 +50:12:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 3.990 357876436250147968 027.57818957523 +50.20866696194 10.3958 9.8902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203931_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203931_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:24.69 +49:45:59.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203933_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203933_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203934_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203934_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:41.26 +50:16:44.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203936_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203936_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 203938_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203938_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203939_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203939_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203940_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203940_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:50.86 +50:35:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 3.697 405809095906985472 024.96351347731 +50.59780681854 10.1073 9.7849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203941_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203941_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:43.67 +50:37:30.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 203942_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203942_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203946_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203946_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:09.38 +48:05:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 1.653 399353966219867008 024.78975590093 +48.09362684904 10.3796 10.0271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203947_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203947_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203949_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203949_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203950_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203950_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:09.48 +50:16:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 2.482 405778343941042560 024.53854037646 +50.27373172708 9.9758 9.2778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203951_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203951_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203952_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203952_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203954_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203954_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 203955_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203955_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203956_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203956_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203958_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203958_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:48.16 +49:05:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 4.988 405426294061579264 024.70277043838 +49.08948119266 10.3224 9.9512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203960_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203960_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203961_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203961_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203963_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203963_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203964_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203964_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:51.31 +50:38:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 4.549 405856374906721536 024.46227818080 +50.63751623852 10.1513 9.3232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203966_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203966_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203969_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203969_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203970_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203970_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:10.34 +47:57:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 5.581 399351423599028224 024.79537521762 +47.95252339166 10.4273 9.9820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203977_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203977_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:33.12 +49:25:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 4.136 357463191676376064 026.63972187943 +49.42532761675 10.7382 10.3001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203978_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203978_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203980_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203980_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203982_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203982_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203983_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203983_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:26.07 +49:37:10.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)
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Considering the candidate 203989_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203989_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203990_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203990_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:33.98 +50:02:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 4.370 405757590659295104 025.14347104815 +50.04846295965 10.5435 10.2985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203994_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 203994_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 203999_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 203999_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:27.34 +50:12:19.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 204004_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204004_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204006_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204006_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204009_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204009_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:50.56 +50:22:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.623 405825863459166080 024.46180126284 +50.36994389500 10.3603 9.9665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204011_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204011_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:24.89 +50:45:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 2.345 405861971246742400 024.60269511792 +50.76150537297 10.2731 9.5367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204015_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204015_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:04.50 +49:28:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 3.529 357827645419647616 027.27025383710 +49.47225598005 10.7223 10.1526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204016_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204016_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:22.05 +47:39:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 3.545 399291289759627008 024.84328251840 +47.66137724918 10.6998 10.2307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204018_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204018_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 204019_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204019_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:31.28 +49:55:01.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)
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Considering the candidate 204020_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204020_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204022_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204022_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204024_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204024_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204025_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204025_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204026_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204026_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:19.39 +50:54:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 4.464 406098198746462720 026.58259455849 +50.91325467432 10.9790 10.6994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204029_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204029_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204030_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204030_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204031_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204031_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204032_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204032_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204034_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204034_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:58.61 +48:17:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 5.866 399380556359876480 024.99628832994 +48.29788795416 10.6443 10.1609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204037_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204037_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 204040_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204040_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204041_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204041_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204044_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204044_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:34.38 +49:04:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 4.635 405422583210000896 024.89520600912 +49.07034655979 10.7464 10.4195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204046_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204046_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:45.94 +41:31:26.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)
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Considering the candidate 204047_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204047_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 204048_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204048_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204050_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204050_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:43.19 +44:50:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 4.426 350293207633001088 025.43154627113 +44.84135515690 10.8878 10.4436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204059_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204059_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204061_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204061_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204063_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204063_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204068_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204068_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 204073_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204073_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:36.08 +44:28:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 5.163 350258813534496896 025.40232740315 +44.47698754321 10.6034 9.9469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204076_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204076_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:08:41.33 +44:28:51.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204077_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204077_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:39.40 +50:14:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.821 405819060231020544 024.41468164317 +50.23955050345 10.7583 10.3743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204078_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204078_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204080_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204080_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204082_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204082_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:50.60 +48:26:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 3.643 399341287476068864 025.21216968296 +48.44323799229 10.9147 10.4226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204084_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204084_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:48.50 +48:49:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 4.071 405403650994227968 025.20379013574 +48.82045724908 10.7997 10.3280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204085_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204085_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204086_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204086_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204087_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204087_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204089_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204089_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204090_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204090_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:04.67 +42:21:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 4.408 347744363582849792 026.02039486476 +42.35442664943 10.8992 10.2262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204091_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204091_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:34.23 +48:19:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 3.928 399339122812582912 025.14416297667 +48.32951972004 10.9773 10.4699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204092_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204092_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204093_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204093_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204096_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204096_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 204097_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204097_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204098_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204098_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204099_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204099_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:52:00.72 +44:52:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.328 433806304081995008 043.00312737053 +44.87759813846 12.5038 12.0780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204100_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204100_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204101_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204101_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204102_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204102_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204103_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204103_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:02.88 +50:22:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 5.584 405791366282042240 025.26443035609 +50.36674508792 10.7130 10.0502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204111_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204111_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:05.95 +50:08:10.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 204113_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204113_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:54.79 +50:24:35.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)
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Considering the candidate 204115_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204115_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:09.95 +47:39:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 3.275 399282356227651200 025.29254668172 +47.65962222731 11.1988 10.7054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204116_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204116_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204118_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204118_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204119_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204119_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204120_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204120_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204122_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204122_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204126_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204126_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:55.07 +49:54:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 4.542 405564626368343936 025.48141625939 +49.91048630171 11.1264 10.6460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204127_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204127_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:05.30 +40:54:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 5.556 347057344910695680 026.02361707999 +40.91674148643 11.1339 10.6194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204136_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204136_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 204137_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204137_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204138_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204138_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204140_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204140_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204141_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204141_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:16.49 +50:07:21.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
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Considering the candidate 204142_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204142_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204148_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204148_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:23.66 +48:39:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 5.833 399405780704771072 024.60100092307 +48.66146898952 11.2049 10.8055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204149_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204149_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204152_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204152_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:34.74 +50:17:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 5.058 405777828543032832 024.64689005694 +50.28637184468 11.0547 10.7168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204153_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204153_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204154_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204154_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204156_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204156_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204157_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204157_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 204158_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204158_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204160_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204160_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204161_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204161_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:06.80 +47:44:28.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)
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Considering the candidate 204162_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204162_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204164_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204164_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204165_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204165_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204168_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204168_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:21.04 +48:43:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 5.561 399409560275979392 024.58997595718 +48.73356377019 10.9824 10.4727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204170_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204170_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204171_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204171_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204172_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204172_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204173_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204173_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204174_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204174_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204176_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204176_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204177_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204177_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204178_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204178_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204179_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204179_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204183_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204183_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:47.33 +50:35:35.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204185_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204185_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204190_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204190_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204191_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204191_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204194_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204194_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204195_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204195_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204197_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204197_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:45.39 +40:59:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 5.710 347243055000069760 025.69080466115 +40.98436973900 11.4351 11.0845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204198_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204198_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 204200_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204200_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204202_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204202_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204205_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204205_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204208_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204208_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204211_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204211_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 204215_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204215_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 204216_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204216_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:29.18 +48:05:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.730 399326989527774720 025.12305297576 +48.08438708647 11.2797 10.8127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204217_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204217_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 204218_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204218_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:58.22 +49:34:17.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 204219_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204219_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204221_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204221_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:15.74 +50:01:45.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 204222_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204222_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:03.21 +49:31:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 4.143 357828916732359168 027.26510271905 +49.51809121116 11.4816 10.9352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.143#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204227_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204227_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 204229_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204229_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204230_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204230_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:29.33 +47:47:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 0.465 354260550526470912 037.62233078406 +47.79148357625 12.9269 12.0689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204231_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204231_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204234_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204234_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204235_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204235_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:08.70 +47:42:05.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 204236_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204236_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:33.37 +42:11:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.663 347776769113838976 026.63994743529 +42.19401500408 11.5142 10.9969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204241_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204241_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:57.55 +50:02:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 5.402 405766180593714560 024.74203473220 +50.04908721651 11.2540 10.7630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204245_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204245_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204247_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204247_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:50:10.69 +48:39:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.878 437827458624597120 042.54487678935 +48.66528628573 13.0626 12.6319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204251_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204251_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204252_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204252_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 204254_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204254_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204255_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204255_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204256_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204256_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:18.22 +42:30:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 5.065 347760860554904576 025.82782184829 +42.51083326376 11.3015 10.6004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204257_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204257_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:04.65 +49:29:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 5.459 405644096147484800 024.77159163656 +49.49978220777 11.4699 11.0461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204258_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204258_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:28.10 +50:54:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 5.813 406018965189180928 026.11961648457 +50.90568007261 11.6976 11.4091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204260_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204260_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:31:46.06 +46:35:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.662 342074491357002624 037.94210413156 +46.59602010641 13.1260 12.3984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204261_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204261_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204262_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204262_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204264_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204264_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:17.53 +45:07:07.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)
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Considering the candidate 204265_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204265_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:24.52 +45:42:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.553 350631376178042624 025.35376321492 +45.70112478588 11.7055 11.2545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204267_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204267_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204268_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204268_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204269_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204269_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204272_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204272_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204276_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204276_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:41:06.15 +47:34:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.159 438084400746710400 040.27593169039 +47.58255233806 13.2602 12.5730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204277_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204277_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204279_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204279_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:31.11 +50:38:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.415 405857229602852608 024.38017029748 +50.64452019919 11.2170 10.7255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204280_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204280_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:28:54.39 +49:35:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.138 450721981239463808 037.22749726346 +49.58795737020 13.0736 12.5726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204282_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204282_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204284_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204284_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204285_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204285_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204289_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204289_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 204291_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204291_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 204293_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204293_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204296_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204296_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204299_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204299_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:55:55.44 +45:49:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.772 433943846114946688 043.98129140413 +45.82387562553 13.1411 12.6717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204300_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204300_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:38.90 +49:29:02.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 204302_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204302_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:24.85 +48:47:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 2.278 405398664534593152 025.10449351545 +48.79094586570 11.5505 11.0253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204303_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204303_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204304_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204304_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204306_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204306_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 204309_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204309_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:03.56 +47:28:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.977 399273255194341376 025.26622530737 +47.48224610508 11.7400 11.0542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204312_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204312_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204313_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204313_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:38.15 +49:36:42.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 204314_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204314_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:44:03.55 +49:15:15.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204315_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204315_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:32.40 +50:24:41.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 204316_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204316_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:14.50 +48:09:25.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 204317_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204317_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204320_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204320_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204321_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204321_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:56.42 +49:57:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.198 405752608497073152 024.73679132191 +49.96035941296 11.6373 11.3174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204322_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204322_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:18.54 +49:55:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 5.588 357857469674457600 026.82957751103 +49.93285070454 11.7107 11.2643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204324_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204324_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204326_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204326_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204327_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204327_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:41.94 +50:38:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.087 405798822345205888 025.17591650133 +50.64196283079 11.4927 11.0003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204330_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204330_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:46.79 +46:00:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.393 341679324301735296 037.44503273290 +46.00090394412 13.3472 12.6368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204332_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204332_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 204334_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204334_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:21.15 +50:21:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.327 405800059295657344 024.83769700686 +50.35089139761 11.3198 10.5949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204335_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204335_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204338_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204338_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:47.71 +44:43:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.645 341446090398464128 036.94839538417 +44.72102912247 13.7358 13.2869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204342_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204342_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204344_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204344_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204345_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204345_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 204354_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204354_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:24.76 +50:32:58.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)
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Considering the candidate 204355_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204355_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204356_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204356_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204357_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204357_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204359_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204359_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204361_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204361_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:12.11 +49:43:29.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 204363_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204363_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204368_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204368_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204370_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204370_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 204371_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204371_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 204373_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204373_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204374_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204374_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 204375_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204375_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204376_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204376_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204381_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204381_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:23.38 +48:24:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.319 399340286746040192 025.09784767433 +48.40447871312 11.7627 11.3111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204383_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204383_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204385_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204385_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204386_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204386_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204388_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204388_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204389_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204389_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:40.04 +41:08:13.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 204391_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204391_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204392_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204392_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204396_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204396_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:22.36 +48:34:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.433 399399557295183232 024.59460351979 +48.57542539264 11.6049 11.1529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204398_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204398_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204399_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204399_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204400_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204400_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204402_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204402_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:52.72 +47:56:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.790 399313284289439488 025.22154695546 +47.94440086125 11.7222 11.1970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204403_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204403_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:23:52.21 +49:19:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.664 355376868363498240 035.96814369694 +49.33253331669 13.5643 12.8524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204404_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204404_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204407_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204407_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:53:30.85 +48:34:27.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204408_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204408_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204409_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204409_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204410_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204410_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204411_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204411_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204413_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204413_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:57.49 +49:08:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.654 405470751265668864 025.99147759304 +49.13463064605 11.9901 11.5107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204414_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204414_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204416_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204416_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 204417_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204417_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204418_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204418_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:32.30 +49:22:52.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 204419_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204419_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:24.77 +50:28:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.454 405830605103017984 024.35141866692 +50.47103878212 11.2895 10.4759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204420_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204420_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204421_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204421_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 204422_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204422_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204423_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204423_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:48.38 +44:28:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.899 350279390720282112 025.45202204837 +44.47829765876 11.8401 11.3507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204424_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204424_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:50.14 +46:57:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.930 351127427720037120 025.21057762995 +46.94992654959 11.8857 11.5007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204425_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204425_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204429_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204429_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:31.43 +45:44:58.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 204434_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204434_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204435_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204435_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204436_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204436_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 204437_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204437_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204439_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204439_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 204442_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204442_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 204445_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204445_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:03.18 +41:20:54.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)
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Considering the candidate 204446_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204446_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:56:46.99 +48:44:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.803 437688434826380032 044.19606760388 +48.73629579901 12.9668 12.1441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204447_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204447_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:54:22.50 +42:35:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.045 336561887948992256 043.59412429453 +42.59257538700 13.1281 12.7263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204448_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204448_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:42:07.12 +44:19:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.134 340691825421723648 040.52964355962 +44.32742579716 13.4934 13.0054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204449_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204449_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204452_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204452_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:38.33 +50:03:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.283 405759751026544256 024.91170791458 +50.06087769723 11.4367 10.7277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204453_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204453_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204454_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204454_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204458_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204458_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:47:07.24 +49:05:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.580 438646904024651904 041.78011717092 +49.09200871922 13.5289 13.3370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204460_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204460_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204466_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204466_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:41:28.15 +40:54:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.177 336722416646595072 040.36767970164 +40.90025575380 12.8593 11.8027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204470_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204470_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:10.29 +50:54:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.949 406098331887822720 026.54459958812 +50.91040905366 11.7970 11.2459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204476_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204476_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204477_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204477_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204482_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204482_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204484_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204484_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 204485_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204485_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204488_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204488_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:19.42 +42:03:18.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)
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Considering the candidate 204490_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204490_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:44.24 +46:00:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 3.318 341679289942273280 037.43391061761 +46.00170977267 14.0031 13.4205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204494_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204494_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:34.04 +49:18:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 5.862 405450071000623360 025.14431003929 +49.31548260399 12.0253 11.6460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204499_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204499_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:09.23 +45:57:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.063 341105791549914752 040.03810901829 +45.95119578160 13.7101 12.9507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204500_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204500_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204501_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204501_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:12.44 +44:50:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 4.521 340582694596163712 039.05360201563 +44.84640345813 13.9168 13.4432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204502_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204502_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204508_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204508_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204510_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204510_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:35:41.28 +43:34:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.997 340367263333508608 038.92211766593 +43.57418015482 13.6370 12.9645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204514_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204514_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204516_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204516_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:05:59.80 +43:36:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.417 432912126251879296 046.49922657389 +43.60294678255 13.0993 12.4915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204518_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204518_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204520_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204520_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 204521_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204521_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 204525_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204525_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204527_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204527_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204528_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204528_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204529_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204529_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 204530_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204530_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:50:54.16 +46:03:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.855 436997327344456192 042.72600331541 +46.06009655825 13.6595 13.1385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204531_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204531_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204533_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204533_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 204536_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204536_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204538_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204538_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204540_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204540_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204542_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204542_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:31.06 +46:36:33.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 204543_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204543_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204544_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204544_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204546_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204546_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 204547_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204547_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:55.07 +47:28:55.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 204550_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204550_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:42.78 +49:22:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.042 357453124273043968 026.93034654795 +49.38099160432 12.1441 11.6765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204551_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204551_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:03:34.38 +48:15:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.454 436112564082783616 045.89347307642 +48.26412554840 13.2732 12.4385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204552_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204552_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:17.83 +48:37:23.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 204553_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204553_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:26.12 +48:26:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 5.818 399385130502231424 024.86021671343 +48.43813564748 11.9514 11.5099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204554_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204554_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:01.17 +41:47:10.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 204555_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204555_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204556_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204556_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:15:48.88 +49:40:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.645 355584195024416640 033.95358887703 +49.67924019060 13.4082 12.8253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204557_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204557_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:43:28.99 +41:51:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.880 336878925254475136 040.87111044299 +41.84999746476 13.5538 13.1065 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.880#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204558_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204558_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:50:05.92 +42:21:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 2.022 337244066194919296 042.52541028523 +42.35882832902 13.3708 12.6676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204560_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204560_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204563_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204563_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:56:33.80 +48:28:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.492 437666998647051904 044.14184608142 +48.48136359426 13.7588 12.9836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204564_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204564_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204565_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204565_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:43.99 +48:51:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.944 405404883647235840 025.18494201172 +48.85728375693 12.1017 11.7559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204567_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204567_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204569_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204569_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204570_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204570_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204572_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204572_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 204574_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204574_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:40.50 +48:15:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.063 399359699998690304 024.67041341022 +48.25875473621 11.7683 11.2222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204575_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204575_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204578_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204578_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:28.20 +46:51:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 3.387 351103478982411648 025.11870929170 +46.85166264584 12.0980 11.6504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204580_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204580_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:09.43 +45:57:07.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 204581_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204581_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:18.33 +50:13:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.164 405775045406171008 024.82652365862 +50.23236454393 11.7196 11.0531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204583_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204583_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204584_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204584_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:29:38.38 +44:38:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.174 341274635303668352 037.40969487582 +44.63681318370 13.9029 13.3974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204585_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204585_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204587_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204587_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204588_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204588_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204589_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204589_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204591_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204591_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:24:15.81 +48:25:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.491 354490455831813120 036.06690329362 +48.43174599761 13.7701 13.1646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204592_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204592_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:51:47.05 +46:49:02.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204594_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204594_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:48:39.03 +43:36:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.439 337632709195694976 042.16305089273 +43.60506000937 13.7399 13.1869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204595_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204595_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204600_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204600_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204601_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204601_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:02.35 +47:47:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 4.529 351269191704823808 025.51164037979 +47.79207784682 12.2861 12.2208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204603_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204603_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:01.58 +48:46:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.257 405354580990288896 025.50668218584 +48.78281515856 12.0984 11.6472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204609_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204609_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204610_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204610_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204613_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204613_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:31.59 +42:55:22.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 204616_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204616_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204617_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204617_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:55.57 +50:03:15.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 204618_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204618_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204623_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204623_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 204625_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204625_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:57.75 +45:59:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.858 341813980116646144 038.49134488611 +45.99882247912 12.4844 10.4705 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204626_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204626_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:28.66 +48:02:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 4.016 399316995141323776 025.62025864738 +48.03749075469 12.4349 11.9382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204627_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204627_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 204628_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204628_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:32.90 +43:25:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.673 340361147299749376 038.63688213778 +43.41766130492 13.8636 13.6939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204629_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204629_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 204633_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204633_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204636_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204636_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:27.84 +50:12:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.356 405817578464757632 024.36577619041 +50.21154292817 11.8169 11.1388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204638_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204638_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:19.30 +48:41:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.471 399395227967685120 024.83058454798 +48.69998292037 12.0648 11.5729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204639_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204639_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204642_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204642_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:06:56.03 +49:38:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.575 358175743930883968 031.73408357360 +49.63352686463 13.3003 12.8166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204643_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204643_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204644_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204644_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204646_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204646_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204648_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204648_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 204649_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204649_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204650_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204650_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204653_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204653_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:13:22.91 +44:12:39.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204654_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204654_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204655_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204655_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204658_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204658_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 204663_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204663_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:06:37.19 +47:45:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.279 356501977995975680 031.65496042095 +47.75224405528 13.6392 13.3367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204665_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204665_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:57.80 +41:50:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 4.035 347716188598660864 025.49232432049 +41.83742623487 12.2557 11.8256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204666_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204666_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:54:52.39 +47:20:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.838 437467604786690432 043.71867288027 +47.33830135274 13.6820 12.9862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204667_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204667_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204669_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204669_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:50:41.35 +47:07:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.945 437123732524262912 042.67288114877 +47.13166774007 13.9378 13.2993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204674_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204674_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:59.33 +50:11:59.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 204676_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204676_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 204681_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204681_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:11:24.59 +44:05:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.766 351780468907242368 032.85256965615 +44.09862707610 13.5775 12.8695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204682_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204682_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204689_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204689_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:42.27 +43:58:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.140 340484189520961664 039.42655428311 +43.97995826101 14.1197 13.3369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204691_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204691_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204692_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204692_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:57:49.83 +45:55:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.640 434130797451957760 044.45787825646 +45.92611467559 13.4545 12.8400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204693_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204693_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204695_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204695_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:27:55.84 +47:09:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.684 354127720073646336 036.98332450871 +47.15988693717 14.4078 13.9188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204699_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204699_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204703_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204703_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:50:45.52 +48:17:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.609 437801551382070656 042.69033359833 +48.28399781817 13.9272 13.3390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204706_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204706_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:16.56 +48:09:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.367 357285757987314688 025.82014911014 +48.15200798259 12.3440 11.8394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204707_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204707_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:43.23 +46:04:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.309 341870227009531264 039.43008242563 +46.07694328376 14.6051 13.5008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204708_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204708_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:46:47.68 +41:09:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.085 336036768067174528 041.69915431880 +41.16014235863 13.8629 13.4353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204709_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204709_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:33.32 +49:51:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.668 405564763807306880 025.39123465508 +49.86271296608 12.2800 11.8056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204711_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204711_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:49.05 +50:57:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.860 406063594192329600 027.45622470769 +50.96340098837 12.5978 12.3108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204713_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204713_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:13.77 +50:07:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 5.165 405591834984385024 025.55960914150 +50.13119504490 12.4780 11.9540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.165#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204715_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204715_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:42:42.82 +46:22:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.637 437206337632451584 040.67904394656 +46.38072317297 14.1225 13.5699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204717_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204717_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:45:15.63 +46:04:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.621 437140744892351744 041.31496276946 +46.08173038420 14.2773 13.6913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204718_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204718_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:48:54.05 +49:10:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.016 438603645114422400 042.22560934132 +49.16784009447 13.9666 13.5940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204719_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204719_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:19.21 +50:53:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.065 406192615010775424 025.08226567549 +50.89405231208 12.2319 11.9417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204720_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204720_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204721_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204721_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:34:35.91 +46:20:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.352 341842258181175552 038.65013909619 +46.33446086162 14.1814 13.7069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204725_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204725_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:37.34 +50:38:19.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
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Considering the candidate 204726_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204726_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 204730_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204730_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:26.40 +41:20:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 5.577 347445197638938368 026.36164586502 +41.33543397593 12.4404 12.0164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204731_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204731_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:46:53.19 +47:14:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 4.906 437351232649701504 041.72362276594 +47.24346531764 14.0661 13.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204733_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204733_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204735_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204735_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 204736_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204736_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:42.58 +46:06:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.146 341870708045860864 039.42760964300 +46.10837220185 14.0983 13.4045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204738_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204738_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:44:04.69 +47:19:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.926 438021831663523840 041.01965063549 +47.32378152574 14.2178 13.6140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204739_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204739_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 204740_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204740_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204744_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204744_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204745_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204745_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 204749_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204749_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 204752_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204752_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204755_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204755_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:02:24.27 +45:04:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 0.061 352774496138367104 030.60114773248 +45.06928290771 13.7079 13.3520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204756_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204756_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204758_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204758_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204759_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204759_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204761_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204761_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 204767_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204767_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204768_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204768_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:02.61 +48:36:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.606 405350801419018496 025.51154314140 +48.60756256797 12.4225 12.0428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204772_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204772_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204773_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204773_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 204774_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204774_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:42.99 +50:43:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.517 405857951157354880 024.42994977808 +50.72302064850 11.8744 11.1526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204776_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204776_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:12.59 +50:13:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.546 405786070586128000 025.05311318783 +50.22993367042 12.2542 11.7786 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204777_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204777_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 204783_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204783_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204784_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204784_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204788_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204788_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 204793_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204793_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204797_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204797_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 204799_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204799_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 204802_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204802_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204805_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204805_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204806_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204806_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:30:00.74 +49:54:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 5.207 450750774700378880 037.50100816225 +49.91013678482 14.2602 13.6536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204812_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204812_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204814_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204814_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 204815_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204815_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:35.54 +49:48:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.816 405747695054679808 024.89967750807 +49.80150414450 12.1346 11.5811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204816_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204816_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:23:20.69 +44:45:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.433 340012808271689984 035.83608073481 +44.76097625214 14.1721 13.6478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204823_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204823_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204826_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204826_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 204827_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204827_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:12:53.92 +43:06:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.220 351411926353263104 033.22515301860 +43.11332916836 14.0400 13.5444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204828_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204828_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204830_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204830_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:52:01.32 +48:44:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.265 437908410168983680 043.00600742889 +48.74111467342 13.9101 13.4852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.265#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204831_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204831_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204833_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204833_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:47:42.04 +48:46:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 4.288 438591069450385280 041.92683906373 +48.76725688802 14.2979 13.7229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204834_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204834_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204835_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204835_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:36:12.87 +45:31:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 0.855 341739350765357952 039.05359742012 +45.52443126866 14.8677 14.1876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204840_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204840_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 204842_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204842_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204846_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204846_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 204848_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204848_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:56.90 +48:18:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.497 405326650820855936 025.73766492713 +48.31235355142 12.4184 11.8646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204852_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204852_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:45.98 +44:36:15.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 204853_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204853_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204855_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204855_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204858_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204858_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:19:08.77 +44:01:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.348 351874026177616512 034.78739353022 +44.02344300757 13.9610 13.3889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204861_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204861_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:51.44 +43:52:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.893 348739112370079360 025.21596785137 +43.86839971670 12.4659 12.0181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204863_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204863_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204866_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204866_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:03.01 +50:04:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.474 405768620135136128 024.51403003619 +50.07185062773 12.1234 11.6137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204867_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204867_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 204868_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204868_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:24.65 +50:21:28.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)
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Considering the candidate 204876_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204876_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:43.58 +47:45:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.050 399293557502356480 024.93182526065 +47.76701788481 12.3320 11.8523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204880_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204880_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:52:41.77 +46:48:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.182 437055459724938624 043.17411751655 +46.80354644656 14.0738 13.5240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204881_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204881_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 204884_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204884_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:10.57 +50:09:41.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
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Considering the candidate 204885_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204885_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 204891_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204891_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204892_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204892_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204893_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204893_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204894_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204894_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:48.05 +41:03:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.108 338389894749901696 038.20022392667 +41.06363860955 14.0724 13.6604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204896_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204896_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204897_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204897_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:03.32 +47:34:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 4.454 399276102755270016 025.26466538909 +47.57021374672 12.3133 11.7235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204898_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204898_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:46.53 +49:00:35.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 204901_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204901_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 204903_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204903_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:49:14.67 +48:15:02.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 204904_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204904_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 204905_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204905_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 204907_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204907_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 204908_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204908_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204911_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204911_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:00:43.53 +46:51:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.497 434466698255955712 045.18171862165 +46.86067637380 13.7640 12.9171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204912_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204912_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 204915_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204915_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204917_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204917_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:59:19.69 +46:08:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.678 355900820013194112 029.83226621452 +46.14507817765 13.4883 12.8157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204918_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204918_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:03.89 +48:54:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.234 438479469019633920 040.01602273831 +48.90379246383 14.2849 13.7875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204919_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204919_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 204920_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204920_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 204922_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204922_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:51.75 +50:57:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 5.851 406053084409963136 026.71783471862 +50.96218814531 12.7311 12.2756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204924_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204924_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 204925_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204925_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204927_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204927_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:03.87 +45:58:38.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)
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Considering the candidate 204930_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204930_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204931_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204931_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:26.98 +49:40:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.813 405652754801546112 024.86318867407 +49.67665912063 12.3156 11.8586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204932_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204932_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204933_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204933_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204934_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204934_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 204935_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204935_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 204936_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204936_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204938_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204938_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204940_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204940_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:40:55.78 +48:04:42.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)
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Considering the candidate 204944_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204944_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:30.13 +50:27:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 4.506 405802322742365824 024.87708098045 +50.45761216577 12.3701 11.8136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204946_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204946_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:00:05.54 +43:29:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.557 432768605624266112 045.02364917316 +43.49350235518 13.8741 13.1906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204948_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204948_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204954_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204954_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204955_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204955_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204957_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204957_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:51.33 +50:23:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.163 405780126351381504 024.71376226568 +50.39831500816 12.2480 11.6781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204962_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204962_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:31:03.18 +48:23:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.391 354349031149313792 037.76303760506 +48.39870449524 14.2245 13.4257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204966_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204966_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:53:21.40 +48:32:28.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 204970_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204970_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:01.67 +50:18:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 4.913 405602044123515904 025.50901243501 +50.30720728319 12.4257 12.0016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204976_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204976_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:11.02 +49:34:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 4.863 405650521418556544 024.79749812090 +49.56807365479 12.4684 12.0140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204978_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204978_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204981_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204981_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 204986_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204986_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 204987_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204987_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 204989_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204989_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:38.66 +50:53:29.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)
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Considering the candidate 204995_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204995_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:21.30 +50:22:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.328 405789235978261248 025.08997616393 +50.37782652522 12.3750 11.8142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204998_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 204998_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:42:47.14 +48:21:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 2.076 438215788088792832 040.69727806079 +48.35618019922 14.1947 13.6901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204999_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 204999_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205000_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205000_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205002_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205002_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205005_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205005_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:37.97 +48:27:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 2.945 399342146469524608 025.15928460640 +48.45681653929 12.5073 11.9681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205006_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205006_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205008_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205008_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:05.74 +49:31:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 4.071 405461267980052224 025.02565281092 +49.52251111647 12.4648 11.9495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205009_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205009_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:07.35 +48:57:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.588 405415745621908608 024.78097810740 +48.96587520065 12.7139 12.4985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205011_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205011_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205017_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205017_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:06.63 +42:52:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.778 338821006387117312 038.27745158686 +42.87596724538 14.3711 13.8932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205018_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205018_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:52.79 +49:13:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 5.441 405448623594164992 024.97225481775 +49.21959240707 12.4882 12.0250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205020_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205020_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 205033_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205033_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205038_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205038_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205039_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205039_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205040_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205040_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205042_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205042_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:17.11 +48:44:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 5.675 399409555979044224 024.57367445672 +48.74037632447 12.5948 12.1498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205045_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205045_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 205046_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205046_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 205047_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205047_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:43:29.27 +41:51:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.803 336879028333689856 040.87288076187 +41.85569941646 14.2531 13.7328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205048_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205048_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:35.14 +43:39:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.334 340404165691954560 038.14698647450 +43.65749968466 14.5458 14.1198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205056_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205056_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:32.83 +50:20:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.407 405820602121728896 024.38782897396 +50.33557457227 12.3427 11.8488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205057_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205057_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:29.23 +50:51:42.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)
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Considering the candidate 205058_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205058_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:45:53.94 +50:47:54.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)
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Considering the candidate 205063_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205063_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205065_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205065_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205066_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205066_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:49:00.90 +41:15:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 4.135 347498661391384448 027.25416548401 +41.26296631790 12.6972 12.1672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205068_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205068_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:47:38.82 +40:53:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.485 336015087072296448 041.91207312252 +40.89322302949 12.3266 10.7579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205072_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205072_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205074_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205074_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 205075_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205075_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:56:46.11 +48:34:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.743 437684900070668032 044.19212768904 +48.56865468681 14.2574 13.6301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205077_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205077_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205083_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205083_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 205085_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205085_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205089_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205089_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205090_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205090_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 205091_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205091_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205094_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205094_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:37.66 +49:56:33.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
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Considering the candidate 205099_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205099_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:02.48 +49:44:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 5.159 405661482175089664 024.51255042467 +49.74755845057 12.0247 11.6181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205100_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205100_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205102_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205102_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205104_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205104_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:27.01 +50:30:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 5.272 405796481586841216 025.11481284025 +50.51136946580 12.3397 11.6762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205109_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205109_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:31:28.96 +41:12:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.032 338444148776416896 037.87092176125 +41.20245364918 14.1764 13.6181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205117_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205117_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:53.98 +41:17:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 5.166 347631015103928960 026.22624055562 +41.29167323730 12.5359 11.9014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205119_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205119_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:30.57 +47:29:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 4.551 351236515595705088 025.37722476021 +47.49464894021 12.2867 11.5746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205126_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205126_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205130_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205130_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:12.00 +48:41:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.962 399406944638468736 024.79997497122 +48.69215001050 12.4462 11.9183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205136_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205136_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 205139_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205139_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:56.58 +42:47:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 2.543 338820113033939712 038.23571783248 +42.79742824730 14.4232 13.9581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205141_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205141_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 205145_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205145_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205147_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205147_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:27.53 +49:48:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 5.094 405888569982824704 026.61687062723 +49.81598594916 12.7649 12.2989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205150_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205150_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205152_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205152_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:45.61 +49:56:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 3.061 405763981570475520 024.69098449942 +49.94481781581 12.2045 11.5421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205153_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205153_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 205158_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205158_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:48:57.90 +41:57:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.207 337209569017754496 042.24155423263 +41.96278031278 14.3114 13.8174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205159_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205159_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:06:07.53 +46:49:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.215 435730243274390528 046.53145592143 +46.83130002068 13.9180 13.3238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205160_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205160_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:41:37.61 +43:06:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.175 337197474388981760 040.40684462535 +43.10828294342 14.5785 13.9755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205162_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205162_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205164_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205164_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205166_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205166_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 205168_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205168_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:09.65 +50:55:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 5.766 406042840910357632 027.04197658952 +50.92576629106 12.9642 12.6919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205169_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205169_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:32.80 +41:09:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 3.337 347262949288577792 025.63706387487 +41.16593298164 12.6711 12.0565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205170_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205170_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:47.93 +40:53:07.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)
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Considering the candidate 205174_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205174_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205175_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205175_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:25.34 +48:13:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.889 399332452726167424 025.10504783906 +48.22544040849 12.6732 12.2111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205178_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205178_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 205182_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205182_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205186_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205186_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205188_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205188_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:04:14.17 +42:15:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.816 240309677981476608 046.05943263441 +42.26702420571 13.7734 13.0594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205189_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205189_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:32.45 +48:23:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 4.212 399395575862531200 024.63661453822 +48.38898271568 12.3815 11.9134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205190_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205190_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205194_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205194_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:56.34 +50:44:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.495 405814932766372864 024.98549861898 +50.73860539343 12.6934 12.4103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205198_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205198_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:11:41.53 +49:15:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.554 436391393360975744 047.92324689406 +49.26156338279 13.5517 12.9092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205203_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205203_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205207_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205207_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205208_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205208_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205212_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205212_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 205213_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205213_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:42.98 +47:56:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 5.636 399346097839384832 024.68077043493 +47.94825021960 12.7496 12.1640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205216_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205216_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205219_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205219_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 205220_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205220_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:04.04 +50:04:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 2.402 405757109622954880 025.01777704608 +50.06847048232 12.5722 12.1634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205224_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205224_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:53.58 +50:18:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 5.530 405779198638449920 024.72536733054 +50.30942308331 12.5133 11.9893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205225_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205225_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 205231_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205231_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205233_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205233_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205234_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205234_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:35.31 +42:42:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 3.556 340082558541573120 039.39662498242 +42.71477813114 14.4502 13.6826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205239_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205239_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:41:17.56 +42:44:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.465 337164970076608512 040.32350808025 +42.73768161312 14.3330 13.6024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205240_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205240_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:59.74 +50:22:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 4.525 405826172696809600 024.50085236044 +50.37193081240 12.2981 11.8264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205241_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205241_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:04:42.19 +47:52:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 2.668 436041851741844096 046.17688215995 +47.87778563185 14.3340 13.5972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205244_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205244_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:47:51.89 +49:18:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 2.417 438655871916219904 041.96704258200 +49.30838404595 14.3938 13.8027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205246_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205246_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:57:35.81 +45:37:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.538 434122722913568000 044.39992237118 +45.63380310939 14.3811 13.6039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205248_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205248_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:39.77 +41:13:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 5.606 347267557790833152 025.66747124414 +41.23292807192 12.6906 12.1732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205253_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205253_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:52:49.06 +50:05:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.292 440247930396483584 043.20465674687 +50.08612963260 13.9160 13.0480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205270_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205270_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:53:12.28 +50:23:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.897 440261502492876672 043.30222203129 +50.39862401970 13.8904 13.1909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205274_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205274_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205282_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205282_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 205284_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205284_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205285_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205285_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:38.69 +50:17:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 5.338 405602353361027968 025.41342277516 +50.28605629718 12.6995 12.2240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205286_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205286_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:02:44.38 +48:21:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 3.677 436116034416336512 045.68613039264 +48.35356779653 14.0324 13.1376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205288_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205288_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205293_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205293_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 205294_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205294_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:07:14.07 +46:42:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 2.727 434980341983551104 046.80972802530 +46.71406908122 14.1478 13.5247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205296_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205296_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:01.60 +49:27:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 4.091 405502263443788544 026.50837478306 +49.45461920917 13.2463 12.8966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205297_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205297_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:17.63 +50:52:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.928 406180730837453312 025.57364837892 +50.88066073997 12.6336 12.0894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205298_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205298_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:48:16.77 +50:55:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 5.314 406042913927414400 027.07089619251 +50.92989395208 13.2286 12.7121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205303_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205303_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:38:42.37 +49:41:10.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)
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Considering the candidate 205305_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205305_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:00.99 +47:57:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 4.402 399311325784502528 025.50594762367 +47.96139890735 13.1465 12.8542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205308_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205308_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:39:01.75 +44:43:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.393 340893929402845568 039.75769885359 +44.72047916122 14.5531 14.1356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205318_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205318_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:15.55 +50:38:21.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)
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Considering the candidate 205325_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205325_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:54.19 +49:34:52.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)
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Considering the candidate 205330_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205330_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205335_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205335_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:51:31.02 +49:32:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.095 438719403073666304 042.87943246986 +49.54339118085 13.9669 12.9869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205336_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205336_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205337_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205337_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 205341_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205341_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205348_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205348_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:10.04 +40:58:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 5.577 347421351980597376 026.54204302356 +40.97931885785 12.4261 11.9387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205349_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205349_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 205357_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205357_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 205364_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205364_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:37:52.86 +50:41:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 4.220 405857126523635072 024.46895646573 +50.69811591056 12.2581 11.5034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205370_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205370_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 205378_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205378_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:49.43 +48:48:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 4.711 405357574585271296 025.45630982499 +48.80634362060 12.9391 12.3992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205381_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205381_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205386_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205386_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:40.25 +43:36:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.089 340403856454317440 038.16769129799 +43.61505213046 14.9683 14.4361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205389_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205389_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:41:06.82 +44:24:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 3.370 350257675365638272 025.27938006855 +44.40280132296 12.9246 12.3585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205392_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205392_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205410_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205410_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205413_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205413_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 205422_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205422_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205425_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205425_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:39:36.13 +49:22:04.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)
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Considering the candidate 205428_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205428_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:44.49 +50:51:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 3.710 406180078002425984 025.68570596056 +50.86179646969 12.7059 12.1842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205431_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205431_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
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Considering the candidate 205432_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205432_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 03:05:47.80 +48:20:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.420 436151356230235776 046.44923720543 +48.34828043175 14.1982 13.5552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205434_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205434_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205435_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205435_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 205439_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205439_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:44:14.10 +50:55:42.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)
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Considering the candidate 205445_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205445_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 205448_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205448_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205452_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205452_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205458_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205458_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:46.92 +50:56:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.283 406204026740060288 025.69577614491 +50.94157794757 12.6386 12.0495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205459_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205459_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:20.21 +50:27:38.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)
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Considering the candidate 205463_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205463_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205464_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205464_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:54.32 +49:58:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 4.562 405896953759051776 026.72819247483 +49.97950366244 12.9964 12.4646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205476_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205476_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205482_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205482_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:38:11.05 +44:18:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.709 340507760302728448 039.54628473759 +44.30310829951 14.7868 14.3480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205489_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205489_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205493_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205493_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205496_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205496_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:53:42.88 +46:32:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.193 434034246586111744 043.42914586509 +46.53965912490 14.5129 13.9171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205504_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205504_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 205505_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205505_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205511_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205511_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205516_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205516_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205522_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205522_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:26.06 +47:49:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 4.356 399299196796739200 025.11027538259 +47.81777714446 12.8225 12.3237 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205525_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205525_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 205532_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205532_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 205534_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205534_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205542_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205542_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205550_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205550_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 205552_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205552_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205556_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205556_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205557_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205557_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 205558_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205558_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205567_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205567_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:40:55.54 +48:08:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 0.553 399328157758875264 025.23131999563 +48.14874933747 12.9153 12.4494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205574_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205574_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 205575_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205575_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 205580_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205580_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:42:25.48 +45:37:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.725 341059990019057152 040.60621334174 +45.62485680664 14.7647 14.2743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205602_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205602_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205607_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205607_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 205614_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205614_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:43:02.81 +49:01:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 4.351 405386398108005760 025.76326182086 +49.02107210522 13.3419 12.9272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205621_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205621_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205626_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205626_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:46:09.38 +41:15:39.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)
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Considering the candidate 205643_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205643_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 205685_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205685_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 205695_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205695_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 205706_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205706_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 205728_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 205728_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:42:21.45 +40:56:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 5.798 347254398011101952 025.59047114946 +40.93682589555 13.5139 13.0898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 205761_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 205761_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 03551_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 03551_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 189665_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 189665_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58280_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 58280_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 157991_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 157991_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:50:17.70 +41:23:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.483 347494744381186560 027.57409554172 +41.39573699810 12.7880 12.2205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140673_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 140673_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 54740_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 54740_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:53.71 +48:20:16.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 115400_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 115400_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 115522_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 115522_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 109055_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 109055_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 159879_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 159879_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 133900_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 133900_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 105213_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 105213_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 118154_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 118154_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 41300_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 41300_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:52:22.70 +48:39:52.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 91447_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 91447_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:32:46.06 +46:29:20.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 97229_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 97229_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:25:49.08 +46:05:19.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)
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Considering the candidate 53026_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 53026_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 34719_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 34719_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:35:51.45 +49:18:00.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 110896_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 110896_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 152856_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 152856_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 24530_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 24530_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50552_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 50552_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 176215_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 176215_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 01:47:32.59 +42:42:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.739 347814221228525824 026.88638588595 +42.71185284550 11.7931 11.2938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 40721_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 40721_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
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Considering the candidate 46191_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
The candidate 46191_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100 did not pass the final checks
**** FOUND 02:11:02.75 +48:56:44.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 172192_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
Preparing report for the candidate 172192_And-03-Q2b1x1_2026-02-21_22-19-53_20.00sec_-14.90C_LIGHT_0100
make_report_in_HTML.sh Phase 2 (HTML assembly): 105s
make_report_in_HTML.sh TOTAL: 1154s
Prepared the HTML report for the field And-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
02:35:51.44 +49:18:00.8
02:52:22.70 +48:39:52.3
02:11:02.76 +48:56:44.2
02:32:53.71 +48:20:16.8
02:32:46.05 +46:29:20.8
01:45:57.46 +49:08:31.1
01:42:50.83 +43:56:33.5
01:42:04.22 +48:01:55.3
01:37:53.07 +50:36:24.1
01:39:31.97 +50:29:42.3
01:44:36.44 +41:10:50.4
01:39:19.25 +49:36:17.6
01:40:52.67 +50:18:02.5
01:38:04.85 +49:25:59.4
01:38:22.85 +49:17:20.3
01:45:30.58 +49:51:02.0
01:39:41.54 +49:00:13.9
01:40:40.90 +50:16:46.3
01:40:24.74 +49:45:59.4
01:40:39.39 +45:07:34.2
01:39:55.75 +46:38:07.0
01:40:43.59 +50:37:31.8
01:41:14.46 +46:52:03.6
01:39:50.16 +50:35:55.4
01:44:21.07 +50:27:44.5
01:37:49.92 +50:22:14.3
01:44:15.38 +42:56:25.3
01:45:27.42 +50:12:18.1
02:25:53.93 +46:25:30.0
01:40:36.95 +50:47:45.7
01:40:05.55 +50:08:11.8
02:56:41.72 +50:33:24.5
02:28:25.37 +45:36:03.5
02:18:55.22 +45:28:22.0
02:33:48.96 +45:12:54.0
02:36:24.20 +44:54:58.7
02:48:15.68 +44:37:04.6
01:45:47.56 +44:49:48.8
02:59:56.11 +42:37:15.3
01:42:11.71 +43:36:15.4
01:44:34.37 +40:54:48.1
01:46:16.24 +41:33:49.5
01:41:47.35 +42:23:36.6
01:46:00.02 +42:35:07.2
01:43:14.67 +42:13:52.2
01:47:31.65 +41:51:38.2
01:45:30.78 +41:03:37.4
01:44:48.85 +41:56:55.0
01:49:01.06 +41:15:55.0
01:44:49.63 +49:57:37.9
01:42:11.64 +48:17:05.0
01:44:15.75 +46:40:34.7
01:43:31.36 +49:36:07.3
02:38:12.61 +47:05:58.4
01:41:50.52 +48:08:44.5
01:42:53.39 +43:50:02.8
01:46:10.89 +50:35:07.3
01:42:16.72 +42:18:43.8
01:46:07.54 +48:37:06.8
01:43:37.26 +44:07:56.8
01:48:15.53 +41:20:03.0
01:41:24.74 +44:25:45.4
01:46:17.19 +45:40:57.6
01:48:29.42 +41:01:54.5
01:49:44.56 +49:53:47.1
01:46:33.45 +43:54:35.7
01:52:40.28 +41:27:03.3
01:43:45.28 +43:49:24.3
01:42:36.23 +48:56:29.8
01:48:59.66 +48:12:09.0
01:44:25.79 +43:43:51.0
01:47:04.56 +47:43:42.6
01:45:11.31 +49:00:15.4
01:44:14.23 +47:19:45.0
01:49:57.88 +49:25:13.3
01:47:23.85 +49:04:34.6
01:43:17.24 +44:50:12.7
01:49:28.57 +41:36:46.3
02:13:12.76 +49:57:24.7
01:47:12.50 +42:46:55.2
01:42:08.85 +48:05:07.3
01:39:05.41 +49:30:51.1
01:41:50.30 +48:40:04.3
01:42:51.28 +47:36:14.0
01:39:39.94 +47:00:40.7
01:38:44.23 +48:52:47.3
01:43:28.37 +42:52:41.6
01:49:50.70 +49:46:20.0
01:44:20.56 +44:14:23.3
01:43:03.01 +45:47:14.3
01:47:08.59 +48:09:21.2
01:59:16.34 +50:55:48.0
01:46:56.64 +43:04:52.0
01:50:45.68 +49:47:12.6
01:44:23.44 +47:33:26.0
01:44:24.54 +43:41:13.4
01:45:29.89 +43:20:45.9
01:47:43.77 +41:03:06.3
01:44:28.02 +45:05:11.2
01:43:42.62 +43:18:01.9
01:41:50.50 +46:01:37.8
01:44:45.60 +43:15:53.0
01:51:11.71 +41:34:55.6
01:44:48.52 +43:53:13.2
01:43:16.49 +45:50:28.8
01:41:20.14 +44:02:27.9
01:45:48.81 +44:58:04.7
01:40:15.25 +46:10:41.1
01:51:13.32 +50:27:20.2
01:42:16.45 +46:55:29.1
01:42:40.68 +42:38:43.6
01:46:08.35 +42:12:53.9
01:51:14.68 +50:50:07.4
01:41:39.06 +48:45:55.3
01:46:14.29 +42:48:52.8
01:44:22.30 +46:13:23.0
01:39:48.75 +47:33:06.6
01:44:10.11 +45:00:10.4
01:48:18.99 +49:06:03.5
01:48:16.75 +42:23:33.7
01:51:15.90 +49:44:40.3
01:42:12.31 +48:06:19.6
01:44:07.77 +43:59:54.7
02:15:26.80 +47:49:30.1
01:39:42.90 +46:08:02.0
01:53:18.35 +50:20:13.6
01:46:55.49 +43:52:12.9
01:44:08.34 +44:31:52.3
01:46:51.96 +48:49:14.8
01:47:43.06 +41:11:40.9
01:45:06.35 +45:11:59.2
01:44:58.59 +44:13:14.9
01:41:56.40 +42:51:51.8
01:42:02.82 +48:01:53.7
01:40:49.45 +47:23:59.4
01:42:41.43 +50:53:46.8
01:43:13.44 +50:03:35.0
01:41:08.64 +47:06:56.6
01:40:00.80 +48:48:14.8
01:39:44.19 +49:12:13.0
01:42:42.91 +46:13:32.6
01:44:04.60 +41:59:53.0
01:41:33.08 +47:09:26.5
01:42:53.94 +42:39:53.6
01:41:24.25 +43:03:13.1
01:45:14.26 +50:43:02.9
01:42:19.97 +46:30:39.4
01:42:25.71 +43:04:53.1
01:43:03.08 +49:14:44.3
01:40:54.32 +45:53:13.6
01:44:36.89 +50:20:54.7
01:48:20.88 +50:22:19.2
01:42:34.81 +46:57:03.4
01:44:23.22 +50:23:38.7
01:40:18.39 +49:31:07.5
01:43:53.92 +42:44:53.9
01:41:48.43 +46:32:32.1
01:48:14.51 +41:15:36.5
01:40:50.14 +44:36:25.6
01:45:17.34 +49:27:14.3
01:46:38.45 +50:55:54.7
01:51:10.81 +50:11:41.3
01:46:26.56 +41:33:31.6
01:47:21.67 +40:56:47.3
01:44:46.48 +50:03:43.0
01:42:40.02 +48:22:31.7
01:41:58.33 +45:40:22.7
01:42:24.03 +47:31:31.3
01:42:11.68 +49:58:09.9
01:44:13.52 +50:47:28.3
01:44:21.12 +42:00:18.3
01:42:55.33 +49:06:37.4
01:47:26.71 +49:57:44.8
01:39:35.57 +49:52:19.9
01:44:35.93 +47:22:04.6
01:44:46.84 +49:40:24.1
01:44:36.47 +41:24:56.4
01:46:55.09 +41:29:32.4
01:44:38.66 +40:54:01.1
01:46:54.82 +50:17:09.6
01:47:08.56 +49:42:19.1
01:45:39.66 +50:02:45.0
01:41:51.60 +46:18:24.2
01:44:52.03 +41:57:29.3
01:47:23.38 +40:55:35.7
01:38:40.54 +48:48:07.7
01:41:00.84 +48:47:27.9
01:41:17.39 +46:27:17.1
01:38:43.41 +47:54:49.2
01:43:19.16 +41:23:19.1
01:39:08.27 +49:01:15.3
01:49:58.89 +50:47:44.2
01:44:56.88 +50:10:28.1
01:47:28.81 +41:22:25.3
01:46:54.10 +41:10:23.1
01:43:10.13 +49:54:13.0
01:40:10.55 +45:21:39.5
01:48:09.36 +50:53:40.7
01:42:50.80 +41:16:19.4
01:41:44.33 +48:56:42.4
01:49:10.98 +50:08:40.1
01:41:13.72 +49:57:03.7
01:41:37.25 +49:31:01.5
01:48:07.32 +50:18:38.5
01:43:50.29 +48:14:20.1
01:42:46.68 +41:03:48.1
01:39:03.62 +47:46:53.4
01:42:37.78 +48:32:05.4
01:40:24.35 +45:31:10.9
01:40:28.67 +50:36:02.1
01:42:31.26 +49:41:32.6
01:42:22.98 +49:10:51.3
01:47:37.68 +41:35:32.3
01:42:18.20 +47:55:50.5
01:42:15.65 +41:22:02.4
01:44:47.49 +41:00:59.5
01:44:37.14 +41:48:38.2
01:47:07.75 +49:19:04.6
01:46:38.82 +41:54:52.4
01:42:10.20 +49:43:57.1
01:41:46.28 +47:10:28.5
01:44:08.29 +50:46:10.9
01:43:05.79 +49:47:23.6
01:44:13.91 +49:20:00.7
01:47:29.28 +41:23:13.3
01:43:19.22 +44:53:54.6
01:46:37.43 +49:51:27.9
01:40:19.18 +48:29:58.1
01:45:53.39 +42:19:49.6
01:40:18.42 +50:12:24.0
01:40:39.60 +50:29:38.0
01:44:12.27 +50:35:01.8
01:47:29.12 +49:53:59.1
01:39:53.62 +46:26:13.6
01:39:54.79 +48:44:41.4
01:42:55.31 +50:35:01.2
01:39:13.66 +47:34:34.4
01:38:57.99 +48:26:44.1
01:40:15.29 +47:01:23.3
01:51:28.58 +50:40:50.0
01:41:47.73 +50:48:42.9
01:41:28.15 +50:45:37.4
01:44:09.59 +48:57:04.9
01:43:00.68 +50:24:37.4
01:40:14.97 +45:31:37.8
01:42:57.72 +42:19:18.6
01:42:50.32 +45:52:17.2
01:43:37.77 +47:25:45.4
01:41:30.75 +43:52:17.3
01:47:08.66 +40:59:47.9
01:42:29.49 +47:16:49.1
01:42:15.76 +41:27:52.2
01:42:51.08 +43:06:44.4
01:43:36.69 +41:13:27.0
01:44:10.00 +41:26:56.9
01:42:55.50 +41:25:28.6
01:46:27.43 +50:15:31.0
01:46:43.96 +41:33:49.0
01:40:58.36 +44:53:38.1
01:43:42.36 +48:22:35.3
01:40:07.54 +47:00:48.3
01:37:53.81 +49:31:02.6
01:41:03.82 +44:44:46.8
01:39:23.28 +50:19:09.9
01:48:08.64 +49:34:01.7
01:44:47.42 +50:21:23.8
01:45:59.06 +40:53:19.0
01:40:05.34 +49:36:51.7
01:44:22.23 +45:26:14.8
01:41:37.79 +45:33:04.7
01:43:29.86 +49:41:03.1
01:44:31.98 +50:40:49.8
01:44:40.03 +41:26:50.8
01:40:10.42 +50:40:29.6
01:38:44.76 +49:37:45.6
01:45:52.22 +48:57:57.0
01:43:32.43 +50:24:35.3
01:37:31.29 +50:24:10.9
01:45:33.11 +50:14:55.2
01:46:42.32 +50:10:12.3
01:44:12.08 +42:09:50.1
01:42:46.71 +48:02:54.1
01:47:07.49 +41:16:33.6
01:45:53.14 +49:31:40.4
01:48:01.76 +49:58:50.0
01:41:34.03 +47:35:43.1
01:39:11.47 +49:22:07.7
01:46:23.83 +50:05:58.0
01:41:39.17 +46:45:57.0
01:38:16.29 +49:36:44.0
01:39:11.32 +47:26:23.9
01:41:39.83 +43:15:07.9
01:41:47.04 +42:49:16.7
01:43:57.46 +44:22:08.2
01:40:01.06 +46:44:49.1
01:45:23.80 +41:52:27.9
01:47:39.04 +41:09:46.3
01:42:35.62 +43:19:12.3
01:41:34.81 +50:04:10.2
01:44:47.62 +47:52:24.7
01:45:47.96 +50:04:49.7
01:45:14.42 +49:04:08.3
01:46:04.17 +42:10:40.0
01:40:10.03 +47:23:35.8
01:45:15.59 +49:25:52.2
01:43:55.65 +43:11:05.6
01:51:13.71 +50:00:48.0
01:43:08.01 +41:05:22.5
01:40:26.75 +50:42:36.7
01:38:52.27 +49:43:52.5
01:41:22.02 +43:22:47.8
01:41:51.87 +44:47:41.4
01:45:00.36 +50:35:25.7
01:41:52.74 +48:30:11.1
01:41:09.12 +50:32:09.1
01:45:13.52 +50:03:38.4
01:41:16.39 +50:02:34.2
01:45:44.25 +48:18:31.2
01:43:03.73 +50:33:40.0
01:46:28.14 +49:35:08.9
01:45:55.88 +50:44:39.8
01:42:35.85 +41:06:58.6
01:50:37.60 +50:34:55.7
01:39:43.63 +46:42:23.2
01:41:31.88 +43:16:12.5
01:41:29.77 +42:45:16.0
01:41:46.39 +44:21:09.3
01:43:12.02 +50:32:39.7
01:43:58.52 +47:40:24.8
01:46:25.78 +41:40:10.5
01:40:20.90 +50:28:37.1
01:44:34.81 +42:55:59.7
01:46:00.65 +50:03:46.1
01:41:56.25 +42:44:53.5
02:22:26.91 +42:18:07.3
01:42:40.09 +41:50:36.9
01:44:48.28 +40:57:58.0
01:38:10.39 +50:22:34.6
01:47:13.39 +50:08:57.4
01:42:02.91 +41:38:42.5
01:41:20.24 +49:23:44.2
01:41:40.64 +50:38:38.2
01:46:40.73 +49:57:41.8
01:56:48.56 +43:10:17.5
01:40:26.67 +49:25:27.3
01:42:45.77 +42:01:56.6
01:41:05.23 +44:36:05.5
01:48:38.44 +50:20:15.2
01:44:30.20 +50:39:18.1
01:45:34.46 +49:47:07.4
01:42:44.88 +50:12:26.3
01:41:52.77 +44:11:18.7
01:48:45.20 +50:33:06.6
01:54:13.09 +50:55:58.7
01:42:51.48 +50:52:29.6
02:18:18.35 +49:53:11.9
01:46:38.46 +41:34:18.3
01:40:33.18 +49:47:52.3
01:39:04.13 +49:43:21.1
01:45:11.61 +49:46:13.1
01:45:19.00 +42:29:43.3
01:42:53.36 +41:42:06.2
01:42:24.83 +43:21:44.5
01:39:29.18 +50:16:33.7
01:53:01.77 +50:59:18.7
01:41:41.33 +49:43:08.2
01:43:37.79 +43:49:53.3
01:43:27.48 +50:28:06.0
01:43:11.97 +44:52:32.4
01:46:10.95 +49:00:54.1
01:38:20.74 +50:37:24.7
01:46:28.51 +49:52:23.4
01:41:32.61 +49:02:41.5
01:44:12.76 +41:15:28.4
01:42:25.29 +41:30:33.2
01:41:32.23 +45:53:25.1
01:45:22.30 +49:57:25.0
01:39:38.57 +48:18:37.7
01:49:03.79 +41:05:49.8
01:40:20.89 +48:05:07.4
01:52:01.75 +50:43:20.4
01:47:27.45 +49:45:10.3
01:43:02.95 +50:49:28.9
01:47:18.94 +49:50:41.9
01:42:20.08 +50:49:16.0
01:43:23.89 +42:07:14.2
01:38:43.91 +48:34:01.6
01:39:18.03 +48:11:10.5
01:43:18.98 +50:21:32.1
01:44:27.99 +50:36:09.1
01:45:47.48 +40:55:31.0
01:41:34.51 +50:12:58.6
01:40:19.08 +50:48:57.1
01:43:41.87 +40:50:33.1
01:42:06.04 +49:51:07.1
01:48:01.18 +40:58:04.6
01:37:53.96 +49:36:12.5
01:39:22.89 +49:33:38.1
01:41:59.00 +49:23:43.8
01:44:27.15 +41:10:32.2
01:38:20.35 +50:37:01.3
01:40:13.36 +49:51:56.8
01:43:17.75 +50:48:53.9
01:39:15.98 +49:06:39.2
01:40:30.40 +47:19:17.1
01:44:46.17 +41:07:25.0
01:45:58.19 +41:00:40.6
01:44:32.18 +50:29:57.3
01:45:07.56 +40:53:48.6
01:39:12.53 +48:41:45.9
01:42:07.84 +50:03:45.1
01:45:19.09 +42:16:51.5
01:38:11.35 +50:28:56.2
01:41:52.76 +43:11:19.5
01:39:50.55 +46:04:05.1
01:41:53.55 +49:30:18.0
01:38:41.14 +48:13:18.4
01:39:14.44 +50:19:46.5
01:43:35.00 +50:17:09.0
01:45:14.37 +40:53:42.7
01:46:24.88 +50:22:00.8
01:37:14.74 +50:41:50.2
01:41:13.93 +50:12:17.6
01:43:48.98 +42:02:42.4
01:40:06.33 +46:27:55.9
01:43:10.86 +49:20:43.3
01:41:40.69 +49:13:48.9
01:42:00.01 +42:10:17.7
01:45:19.84 +41:07:56.5
01:44:56.77 +48:16:07.7
01:46:04.56 +40:54:34.9
01:39:21.30 +49:18:05.4
01:44:04.71 +50:31:10.7
01:40:47.42 +49:33:53.7
01:38:12.28 +49:40:34.7
01:41:31.22 +50:15:16.3
01:47:32.15 +41:04:11.7
01:43:43.30 +41:17:08.3
01:42:51.60 +41:39:26.6
01:43:01.94 +43:18:08.2
01:46:43.80 +41:23:12.3
01:42:41.60 +41:01:11.6
01:45:17.70 +41:05:12.1
01:45:18.13 +42:02:14.0
01:44:14.83 +49:40:51.5
01:44:33.13 +41:50:18.8
01:41:35.59 +43:18:35.1
02:32:11.23 +49:54:37.5
01:43:52.46 +48:56:35.1
02:33:46.26 +48:29:08.9
01:40:54.69 +48:17:03.5
02:23:03.21 +48:12:01.7
########### Completed And-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
01:45:57.46 +49:08:31.1
01:42:50.83 +43:56:33.5
01:42:04.22 +48:01:55.3
01:37:53.07 +50:36:24.1
01:39:31.97 +50:29:42.3
01:44:36.44 +41:10:50.4
01:39:19.25 +49:36:17.6
01:40:52.67 +50:18:02.5
01:38:04.85 +49:25:59.4
01:38:22.85 +49:17:20.3
01:45:30.58 +49:51:02.0
01:39:41.54 +49:00:13.9
01:40:40.90 +50:16:46.3
01:40:24.74 +49:45:59.4
01:40:39.39 +45:07:34.2
01:39:55.75 +46:38:07.0
01:40:43.59 +50:37:31.8
01:41:14.46 +46:52:03.6
01:39:50.16 +50:35:55.4
01:44:21.07 +50:27:44.5
01:37:49.92 +50:22:14.3
01:44:15.38 +42:56:25.3
01:45:27.42 +50:12:18.1
02:25:53.93 +46:25:30.0
01:40:36.95 +50:47:45.7
01:40:05.55 +50:08:11.8
02:11:02.76 +48:56:44.2
02:32:53.71 +48:20:16.8
02:52:22.70 +48:39:52.3
02:35:51.44 +49:18:00.8
02:32:46.05 +46:29:20.8
01:43:14.67 +42:13:52.2
01:47:31.65 +41:51:38.2
01:45:30.78 +41:03:37.4
01:44:48.85 +41:56:55.0
01:49:01.06 +41:15:55.0
01:44:49.63 +49:57:37.9
01:42:11.64 +48:17:05.0
01:44:15.75 +46:40:34.7
01:43:31.36 +49:36:07.3
02:38:12.61 +47:05:58.4
01:41:50.52 +48:08:44.5
01:42:53.39 +43:50:02.8
01:46:10.89 +50:35:07.3
01:42:16.72 +42:18:43.8
01:46:07.54 +48:37:06.8
01:43:37.26 +44:07:56.8
01:48:15.53 +41:20:03.0
01:41:24.74 +44:25:45.4
01:46:17.19 +45:40:57.6
01:48:29.42 +41:01:54.5
01:49:44.56 +49:53:47.1
01:46:33.45 +43:54:35.7
01:52:40.28 +41:27:03.3
01:43:45.28 +43:49:24.3
01:42:36.23 +48:56:29.8
01:48:59.66 +48:12:09.0
01:44:25.79 +43:43:51.0
01:47:04.56 +47:43:42.6
01:45:11.31 +49:00:15.4
01:44:14.23 +47:19:45.0
01:49:57.88 +49:25:13.3
01:47:23.85 +49:04:34.6
01:43:17.24 +44:50:12.7
01:49:28.57 +41:36:46.3
02:13:12.76 +49:57:24.7
01:47:12.50 +42:46:55.2
01:42:08.85 +48:05:07.3
01:39:05.41 +49:30:51.1
01:41:50.30 +48:40:04.3
01:42:51.28 +47:36:14.0
01:39:39.94 +47:00:40.7
01:38:44.23 +48:52:47.3
01:43:28.37 +42:52:41.6
01:49:50.70 +49:46:20.0
01:44:20.56 +44:14:23.3
01:43:03.01 +45:47:14.3
01:47:08.59 +48:09:21.2
01:59:16.34 +50:55:48.0
01:46:56.64 +43:04:52.0
01:50:45.68 +49:47:12.6
01:44:23.44 +47:33:26.0
01:44:24.54 +43:41:13.4
01:45:29.89 +43:20:45.9
01:47:43.77 +41:03:06.3
01:44:28.02 +45:05:11.2
01:43:42.62 +43:18:01.9
01:41:50.50 +46:01:37.8
01:44:45.60 +43:15:53.0
01:51:11.71 +41:34:55.6
01:44:48.52 +43:53:13.2
01:43:16.49 +45:50:28.8
01:41:20.14 +44:02:27.9
01:45:48.81 +44:58:04.7
01:40:15.25 +46:10:41.1
01:51:13.32 +50:27:20.2
01:42:16.45 +46:55:29.1
01:42:40.68 +42:38:43.6
01:46:08.35 +42:12:53.9
01:51:14.68 +50:50:07.4
01:41:39.06 +48:45:55.3
01:46:14.29 +42:48:52.8
01:44:22.30 +46:13:23.0
01:39:48.75 +47:33:06.6
01:44:10.11 +45:00:10.4
01:48:18.99 +49:06:03.5
01:48:16.75 +42:23:33.7
01:51:15.90 +49:44:40.3
01:42:12.31 +48:06:19.6
01:44:07.77 +43:59:54.7
02:15:26.80 +47:49:30.1
01:39:42.90 +46:08:02.0
01:53:18.35 +50:20:13.6
01:46:55.49 +43:52:12.9
01:44:08.34 +44:31:52.3
01:46:51.96 +48:49:14.8
01:47:43.06 +41:11:40.9
01:45:06.35 +45:11:59.2
01:44:58.59 +44:13:14.9
01:41:56.40 +42:51:51.8
01:42:02.82 +48:01:53.7
01:40:49.45 +47:23:59.4
01:42:41.43 +50:53:46.8
01:43:13.44 +50:03:35.0
01:41:08.64 +47:06:56.6
01:40:00.80 +48:48:14.8
01:39:44.19 +49:12:13.0
01:42:42.91 +46:13:32.6
01:44:04.60 +41:59:53.0
01:41:33.08 +47:09:26.5
01:42:53.94 +42:39:53.6
01:41:24.25 +43:03:13.1
01:45:14.26 +50:43:02.9
01:42:19.97 +46:30:39.4
01:42:25.71 +43:04:53.1
01:43:03.08 +49:14:44.3
01:40:54.32 +45:53:13.6
01:44:36.89 +50:20:54.7
01:48:20.88 +50:22:19.2
01:42:34.81 +46:57:03.4
01:44:23.22 +50:23:38.7
01:40:18.39 +49:31:07.5
01:43:53.92 +42:44:53.9
01:41:48.43 +46:32:32.1
01:48:14.51 +41:15:36.5
01:40:50.14 +44:36:25.6
01:45:17.34 +49:27:14.3
01:46:38.45 +50:55:54.7
01:51:10.81 +50:11:41.3
01:46:26.56 +41:33:31.6
01:47:21.67 +40:56:47.3
01:44:46.48 +50:03:43.0
01:42:40.02 +48:22:31.7
01:41:58.33 +45:40:22.7
01:42:24.03 +47:31:31.3
01:42:11.68 +49:58:09.9
01:44:13.52 +50:47:28.3
01:44:21.12 +42:00:18.3
01:42:55.33 +49:06:37.4
01:47:26.71 +49:57:44.8
01:39:35.57 +49:52:19.9
01:44:35.93 +47:22:04.6
01:44:46.84 +49:40:24.1
01:44:36.47 +41:24:56.4
01:46:55.09 +41:29:32.4
01:44:38.66 +40:54:01.1
01:46:54.82 +50:17:09.6
01:47:08.56 +49:42:19.1
01:45:39.66 +50:02:45.0
01:41:51.60 +46:18:24.2
01:44:52.03 +41:57:29.3
01:47:23.38 +40:55:35.7
01:38:40.54 +48:48:07.7
01:41:00.84 +48:47:27.9
01:41:17.39 +46:27:17.1
01:38:43.41 +47:54:49.2
01:43:19.16 +41:23:19.1
01:39:08.27 +49:01:15.3
01:49:58.89 +50:47:44.2
01:44:56.88 +50:10:28.1
01:47:28.81 +41:22:25.3
01:46:54.10 +41:10:23.1
01:43:10.13 +49:54:13.0
01:40:10.55 +45:21:39.5
01:48:09.36 +50:53:40.7
01:42:50.80 +41:16:19.4
01:41:44.33 +48:56:42.4
01:49:10.98 +50:08:40.1
01:41:13.72 +49:57:03.7
01:41:37.25 +49:31:01.5
01:48:07.32 +50:18:38.5
01:43:50.29 +48:14:20.1
01:42:46.68 +41:03:48.1
01:39:03.62 +47:46:53.4
01:42:37.78 +48:32:05.4
01:40:24.35 +45:31:10.9
01:40:28.67 +50:36:02.1
01:42:31.26 +49:41:32.6
01:42:22.98 +49:10:51.3
01:47:37.68 +41:35:32.3
01:42:18.20 +47:55:50.5
01:42:15.65 +41:22:02.4
01:44:47.49 +41:00:59.5
01:44:37.14 +41:48:38.2
01:47:07.75 +49:19:04.6
01:46:38.82 +41:54:52.4
01:42:10.20 +49:43:57.1
01:41:46.28 +47:10:28.5
01:44:08.29 +50:46:10.9
01:43:05.79 +49:47:23.6
01:44:13.91 +49:20:00.7
01:47:29.28 +41:23:13.3
01:43:19.22 +44:53:54.6
01:46:37.43 +49:51:27.9
01:40:19.18 +48:29:58.1
01:45:53.39 +42:19:49.6
01:40:18.42 +50:12:24.0
01:40:39.60 +50:29:38.0
01:44:12.27 +50:35:01.8
01:47:29.12 +49:53:59.1
01:39:53.62 +46:26:13.6
01:39:54.79 +48:44:41.4
01:42:55.31 +50:35:01.2
01:39:13.66 +47:34:34.4
01:38:57.99 +48:26:44.1
01:40:15.29 +47:01:23.3
01:51:28.58 +50:40:50.0
01:41:47.73 +50:48:42.9
01:41:28.15 +50:45:37.4
01:44:09.59 +48:57:04.9
01:43:00.68 +50:24:37.4
01:40:14.97 +45:31:37.8
01:42:57.72 +42:19:18.6
01:42:50.32 +45:52:17.2
01:43:37.77 +47:25:45.4
01:41:30.75 +43:52:17.3
01:47:08.66 +40:59:47.9
01:42:29.49 +47:16:49.1
01:42:15.76 +41:27:52.2
01:42:51.08 +43:06:44.4
01:43:36.69 +41:13:27.0
01:44:10.00 +41:26:56.9
01:42:55.50 +41:25:28.6
01:46:27.43 +50:15:31.0
01:46:43.96 +41:33:49.0
01:40:58.36 +44:53:38.1
01:43:42.36 +48:22:35.3
01:40:07.54 +47:00:48.3
01:37:53.81 +49:31:02.6
01:41:03.82 +44:44:46.8
01:39:23.28 +50:19:09.9
01:48:08.64 +49:34:01.7
01:44:47.42 +50:21:23.8
01:45:59.06 +40:53:19.0
01:40:05.34 +49:36:51.7
01:44:22.23 +45:26:14.8
01:41:37.79 +45:33:04.7
01:43:29.86 +49:41:03.1
01:44:31.98 +50:40:49.8
01:44:40.03 +41:26:50.8
01:40:10.42 +50:40:29.6
01:38:44.76 +49:37:45.6
01:45:52.22 +48:57:57.0
01:43:32.43 +50:24:35.3
01:37:31.29 +50:24:10.9
01:45:33.11 +50:14:55.2
01:46:42.32 +50:10:12.3
01:44:12.08 +42:09:50.1
01:42:46.71 +48:02:54.1
01:47:07.49 +41:16:33.6
01:45:53.14 +49:31:40.4
01:48:01.76 +49:58:50.0
01:41:34.03 +47:35:43.1
01:39:11.47 +49:22:07.7
01:46:23.83 +50:05:58.0
01:41:39.17 +46:45:57.0
01:38:16.29 +49:36:44.0
01:39:11.32 +47:26:23.9
01:41:39.83 +43:15:07.9
01:41:47.04 +42:49:16.7
01:43:57.46 +44:22:08.2
01:40:01.06 +46:44:49.1
01:45:23.80 +41:52:27.9
01:47:39.04 +41:09:46.3
01:42:35.62 +43:19:12.3
01:41:34.81 +50:04:10.2
01:44:47.62 +47:52:24.7
01:45:47.96 +50:04:49.7
01:45:14.42 +49:04:08.3
01:46:04.17 +42:10:40.0
01:40:10.03 +47:23:35.8
01:45:15.59 +49:25:52.2
01:43:55.65 +43:11:05.6
01:51:13.71 +50:00:48.0
01:43:08.01 +41:05:22.5
01:40:26.75 +50:42:36.7
01:38:52.27 +49:43:52.5
01:41:22.02 +43:22:47.8
01:41:51.87 +44:47:41.4
01:45:00.36 +50:35:25.7
01:41:52.74 +48:30:11.1
01:41:09.12 +50:32:09.1
01:45:13.52 +50:03:38.4
01:41:16.39 +50:02:34.2
01:45:44.25 +48:18:31.2
01:43:03.73 +50:33:40.0
01:46:28.14 +49:35:08.9
01:45:55.88 +50:44:39.8
01:42:35.85 +41:06:58.6
01:50:37.60 +50:34:55.7
01:39:43.63 +46:42:23.2
01:41:31.88 +43:16:12.5
01:41:29.77 +42:45:16.0
01:41:46.39 +44:21:09.3
01:43:12.02 +50:32:39.7
01:43:58.52 +47:40:24.8
01:46:25.78 +41:40:10.5
01:40:20.90 +50:28:37.1
01:44:34.81 +42:55:59.7
01:46:00.65 +50:03:46.1
01:41:56.25 +42:44:53.5
02:22:26.91 +42:18:07.3
01:42:40.09 +41:50:36.9
01:44:48.28 +40:57:58.0
01:38:10.39 +50:22:34.6
01:47:13.39 +50:08:57.4
01:42:02.91 +41:38:42.5
01:41:20.24 +49:23:44.2
01:41:40.64 +50:38:38.2
01:46:40.73 +49:57:41.8
01:56:48.56 +43:10:17.5
01:40:26.67 +49:25:27.3
01:42:45.77 +42:01:56.6
01:41:05.23 +44:36:05.5
01:48:38.44 +50:20:15.2
01:44:30.20 +50:39:18.1
01:45:34.46 +49:47:07.4
01:42:44.88 +50:12:26.3
01:41:52.77 +44:11:18.7
01:48:45.20 +50:33:06.6
01:54:13.09 +50:55:58.7
01:42:51.48 +50:52:29.6
02:18:18.35 +49:53:11.9
01:46:38.46 +41:34:18.3
01:40:33.18 +49:47:52.3
01:39:04.13 +49:43:21.1
01:45:11.61 +49:46:13.1
01:45:19.00 +42:29:43.3
01:42:53.36 +41:42:06.2
01:42:24.83 +43:21:44.5
01:39:29.18 +50:16:33.7
01:53:01.77 +50:59:18.7
01:41:41.33 +49:43:08.2
01:43:37.79 +43:49:53.3
01:43:27.48 +50:28:06.0
01:43:11.97 +44:52:32.4
01:46:10.95 +49:00:54.1
01:38:20.74 +50:37:24.7
01:46:28.51 +49:52:23.4
01:41:32.61 +49:02:41.5
01:44:12.76 +41:15:28.4
01:42:25.29 +41:30:33.2
01:41:32.23 +45:53:25.1
01:45:22.30 +49:57:25.0
01:39:38.57 +48:18:37.7
01:49:03.79 +41:05:49.8
01:40:20.89 +48:05:07.4
01:52:01.75 +50:43:20.4
01:47:27.45 +49:45:10.3
01:43:02.95 +50:49:28.9
01:47:18.94 +49:50:41.9
01:42:20.08 +50:49:16.0
01:43:23.89 +42:07:14.2
01:38:43.91 +48:34:01.6
01:39:18.03 +48:11:10.5
01:43:18.98 +50:21:32.1
01:44:27.99 +50:36:09.1
01:45:47.48 +40:55:31.0
01:41:34.51 +50:12:58.6
01:40:19.08 +50:48:57.1
01:43:41.87 +40:50:33.1
01:42:06.04 +49:51:07.1
01:48:01.18 +40:58:04.6
01:37:53.96 +49:36:12.5
01:39:22.89 +49:33:38.1
01:41:59.00 +49:23:43.8
01:44:27.15 +41:10:32.2
01:38:20.35 +50:37:01.3
01:40:13.36 +49:51:56.8
01:43:17.75 +50:48:53.9
01:39:15.98 +49:06:39.2
01:40:30.40 +47:19:17.1
01:44:46.17 +41:07:25.0
01:45:58.19 +41:00:40.6
01:44:32.18 +50:29:57.3
01:45:07.56 +40:53:48.6
01:39:12.53 +48:41:45.9
01:42:07.84 +50:03:45.1
01:45:19.09 +42:16:51.5
01:38:11.35 +50:28:56.2
01:41:52.76 +43:11:19.5
01:39:50.55 +46:04:05.1
01:41:53.55 +49:30:18.0
01:38:41.14 +48:13:18.4
01:39:14.44 +50:19:46.5
01:43:35.00 +50:17:09.0
01:45:14.37 +40:53:42.7
01:46:24.88 +50:22:00.8
01:37:14.74 +50:41:50.2
01:41:13.93 +50:12:17.6
01:43:48.98 +42:02:42.4
01:40:06.33 +46:27:55.9
01:43:10.86 +49:20:43.3
01:41:40.69 +49:13:48.9
01:42:00.01 +42:10:17.7
01:45:19.84 +41:07:56.5
01:44:56.77 +48:16:07.7
01:46:04.56 +40:54:34.9
01:39:21.30 +49:18:05.4
01:44:04.71 +50:31:10.7
01:40:47.42 +49:33:53.7
01:38:12.28 +49:40:34.7
01:41:31.22 +50:15:16.3
01:47:32.15 +41:04:11.7
01:43:43.30 +41:17:08.3
01:42:51.60 +41:39:26.6
01:43:01.94 +43:18:08.2
01:46:43.80 +41:23:12.3
01:42:41.60 +41:01:11.6
01:45:17.70 +41:05:12.1
01:45:18.13 +42:02:14.0
01:44:14.83 +49:40:51.5
01:44:33.13 +41:50:18.8
01:41:35.59 +43:18:35.1
02:56:41.72 +50:33:24.5
01:46:00.02 +42:35:07.2
02:23:03.21 +48:12:01.7
01:42:11.71 +43:36:15.4
02:36:24.20 +44:54:58.7
02:48:15.68 +44:37:04.6
02:18:55.22 +45:28:22.0
01:46:16.24 +41:33:49.5
02:59:56.11 +42:37:15.3
02:28:25.37 +45:36:03.5
01:45:47.56 +44:49:48.8
01:40:54.69 +48:17:03.5
02:33:48.96 +45:12:54.0
01:44:34.37 +40:54:48.1
02:32:11.23 +49:54:37.5
02:33:46.26 +48:29:08.9
01:43:52.46 +48:56:35.1
01:41:47.35 +42:23:36.6
###################################################################################
01:45:57.46 +49:08:31.1 -- not an asteroid (will add it to exclusion list)
01:42:50.83 +43:56:33.5 -- not an asteroid (will add it to exclusion list)
01:42:04.22 +48:01:55.3 -- not an asteroid (will add it to exclusion list)
01:37:53.07 +50:36:24.1 -- not an asteroid (will add it to exclusion list)
01:39:31.97 +50:29:42.3 -- not an asteroid (will add it to exclusion list)
01:44:36.44 +41:10:50.4 -- not an asteroid (will add it to exclusion list)
01:39:19.25 +49:36:17.6 -- not an asteroid (will add it to exclusion list)
01:40:52.67 +50:18:02.5 -- not an asteroid (will add it to exclusion list)
01:38:04.85 +49:25:59.4 -- not an asteroid (will add it to exclusion list)
01:38:22.85 +49:17:20.3 -- not an asteroid (will add it to exclusion list)
01:45:30.58 +49:51:02.0 -- not an asteroid (will add it to exclusion list)
01:39:41.54 +49:00:13.9 -- not an asteroid (will add it to exclusion list)
01:40:40.90 +50:16:46.3 -- not an asteroid (will add it to exclusion list)
01:40:24.74 +49:45:59.4 -- not an asteroid (will add it to exclusion list)
01:40:39.39 +45:07:34.2 -- not an asteroid (will add it to exclusion list)
01:39:55.75 +46:38:07.0 -- not an asteroid (will add it to exclusion list)
01:40:43.59 +50:37:31.8 -- not an asteroid (will add it to exclusion list)
01:41:14.46 +46:52:03.6 -- not an asteroid (will add it to exclusion list)
01:39:50.16 +50:35:55.4 -- not an asteroid (will add it to exclusion list)
01:44:21.07 +50:27:44.5 -- not an asteroid (will add it to exclusion list)
01:37:49.92 +50:22:14.3 -- not an asteroid (will add it to exclusion list)
01:44:15.38 +42:56:25.3 -- not an asteroid (will add it to exclusion list)
01:45:27.42 +50:12:18.1 -- not an asteroid (will add it to exclusion list)
02:25:53.93 +46:25:30.0 -- not an asteroid (will add it to exclusion list)
01:40:36.95 +50:47:45.7 -- not an asteroid (will add it to exclusion list)
01:40:05.55 +50:08:11.8 -- not an asteroid (will add it to exclusion list)
02:11:02.76 +48:56:44.2 -- not an asteroid (will add it to exclusion list)
02:32:53.71 +48:20:16.8 -- not an asteroid (will add it to exclusion list)
02:52:22.70 +48:39:52.3 -- not an asteroid (will add it to exclusion list)
02:35:51.44 +49:18:00.8 -- not an asteroid (will add it to exclusion list)
02:32:46.05 +46:29:20.8 -- not an asteroid (will add it to exclusion list)
01:43:14.67 +42:13:52.2 -- not an asteroid (will add it to exclusion list)
01:47:31.65 +41:51:38.2 -- not an asteroid (will add it to exclusion list)
01:45:30.78 +41:03:37.4 -- not an asteroid (will add it to exclusion list)
01:44:48.85 +41:56:55.0 -- not an asteroid (will add it to exclusion list)
01:49:01.06 +41:15:55.0 -- not an asteroid (will add it to exclusion list)
01:44:49.63 +49:57:37.9 -- not an asteroid (will add it to exclusion list)
01:42:11.64 +48:17:05.0 -- not an asteroid (will add it to exclusion list)
01:44:15.75 +46:40:34.7 -- not an asteroid (will add it to exclusion list)
01:43:31.36 +49:36:07.3 -- not an asteroid (will add it to exclusion list)
02:38:12.61 +47:05:58.4 -- not an asteroid (will add it to exclusion list)
01:41:50.52 +48:08:44.5 -- not an asteroid (will add it to exclusion list)
01:42:53.39 +43:50:02.8 -- not an asteroid (will add it to exclusion list)
01:46:10.89 +50:35:07.3 -- not an asteroid (will add it to exclusion list)
01:42:16.72 +42:18:43.8 -- not an asteroid (will add it to exclusion list)
01:46:07.54 +48:37:06.8 -- not an asteroid (will add it to exclusion list)
01:43:37.26 +44:07:56.8 -- not an asteroid (will add it to exclusion list)
01:48:15.53 +41:20:03.0 -- not an asteroid (will add it to exclusion list)
01:41:24.74 +44:25:45.4 -- not an asteroid (will add it to exclusion list)
01:46:17.19 +45:40:57.6 -- not an asteroid (will add it to exclusion list)
01:48:29.42 +41:01:54.5 -- not an asteroid (will add it to exclusion list)
01:49:44.56 +49:53:47.1 -- not an asteroid (will add it to exclusion list)
01:46:33.45 +43:54:35.7 -- not an asteroid (will add it to exclusion list)
01:52:40.28 +41:27:03.3 -- not an asteroid (will add it to exclusion list)
01:43:45.28 +43:49:24.3 -- not an asteroid (will add it to exclusion list)
01:42:36.23 +48:56:29.8 -- not an asteroid (will add it to exclusion list)
01:48:59.66 +48:12:09.0 -- not an asteroid (will add it to exclusion list)
01:44:25.79 +43:43:51.0 -- not an asteroid (will add it to exclusion list)
01:47:04.56 +47:43:42.6 -- not an asteroid (will add it to exclusion list)
01:45:11.31 +49:00:15.4 -- not an asteroid (will add it to exclusion list)
01:44:14.23 +47:19:45.0 -- not an asteroid (will add it to exclusion list)
01:49:57.88 +49:25:13.3 -- not an asteroid (will add it to exclusion list)
01:47:23.85 +49:04:34.6 -- not an asteroid (will add it to exclusion list)
01:43:17.24 +44:50:12.7 -- not an asteroid (will add it to exclusion list)
01:49:28.57 +41:36:46.3 -- not an asteroid (will add it to exclusion list)
02:13:12.76 +49:57:24.7 -- not an asteroid (will add it to exclusion list)
01:47:12.50 +42:46:55.2 -- not an asteroid (will add it to exclusion list)
01:42:08.85 +48:05:07.3 -- not an asteroid (will add it to exclusion list)
01:39:05.41 +49:30:51.1 -- not an asteroid (will add it to exclusion list)
01:41:50.30 +48:40:04.3 -- not an asteroid (will add it to exclusion list)
01:42:51.28 +47:36:14.0 -- not an asteroid (will add it to exclusion list)
01:39:39.94 +47:00:40.7 -- not an asteroid (will add it to exclusion list)
01:38:44.23 +48:52:47.3 -- not an asteroid (will add it to exclusion list)
01:43:28.37 +42:52:41.6 -- not an asteroid (will add it to exclusion list)
01:49:50.70 +49:46:20.0 -- not an asteroid (will add it to exclusion list)
01:44:20.56 +44:14:23.3 -- not an asteroid (will add it to exclusion list)
01:43:03.01 +45:47:14.3 -- not an asteroid (will add it to exclusion list)
01:47:08.59 +48:09:21.2 -- not an asteroid (will add it to exclusion list)
01:59:16.34 +50:55:48.0 -- not an asteroid (will add it to exclusion list)
01:46:56.64 +43:04:52.0 -- not an asteroid (will add it to exclusion list)
01:50:45.68 +49:47:12.6 -- not an asteroid (will add it to exclusion list)
01:44:23.44 +47:33:26.0 -- not an asteroid (will add it to exclusion list)
01:44:24.54 +43:41:13.4 -- not an asteroid (will add it to exclusion list)
01:45:29.89 +43:20:45.9 -- not an asteroid (will add it to exclusion list)
01:47:43.77 +41:03:06.3 -- not an asteroid (will add it to exclusion list)
01:44:28.02 +45:05:11.2 -- not an asteroid (will add it to exclusion list)
01:43:42.62 +43:18:01.9 -- not an asteroid (will add it to exclusion list)
01:41:50.50 +46:01:37.8 -- not an asteroid (will add it to exclusion list)
01:44:45.60 +43:15:53.0 -- not an asteroid (will add it to exclusion list)
01:51:11.71 +41:34:55.6 -- not an asteroid (will add it to exclusion list)
01:44:48.52 +43:53:13.2 -- not an asteroid (will add it to exclusion list)
01:43:16.49 +45:50:28.8 -- not an asteroid (will add it to exclusion list)
01:41:20.14 +44:02:27.9 -- not an asteroid (will add it to exclusion list)
01:45:48.81 +44:58:04.7 -- not an asteroid (will add it to exclusion list)
01:40:15.25 +46:10:41.1 -- not an asteroid (will add it to exclusion list)
01:51:13.32 +50:27:20.2 -- not an asteroid (will add it to exclusion list)
01:42:16.45 +46:55:29.1 -- not an asteroid (will add it to exclusion list)
01:42:40.68 +42:38:43.6 -- not an asteroid (will add it to exclusion list)
01:46:08.35 +42:12:53.9 -- not an asteroid (will add it to exclusion list)
01:51:14.68 +50:50:07.4 -- not an asteroid (will add it to exclusion list)
01:41:39.06 +48:45:55.3 -- not an asteroid (will add it to exclusion list)
01:46:14.29 +42:48:52.8 -- not an asteroid (will add it to exclusion list)
01:44:22.30 +46:13:23.0 -- not an asteroid (will add it to exclusion list)
01:39:48.75 +47:33:06.6 -- not an asteroid (will add it to exclusion list)
01:44:10.11 +45:00:10.4 -- not an asteroid (will add it to exclusion list)
01:48:18.99 +49:06:03.5 -- not an asteroid (will add it to exclusion list)
01:48:16.75 +42:23:33.7 -- not an asteroid (will add it to exclusion list)
01:51:15.90 +49:44:40.3 -- not an asteroid (will add it to exclusion list)
01:42:12.31 +48:06:19.6 -- not an asteroid (will add it to exclusion list)
01:44:07.77 +43:59:54.7 -- not an asteroid (will add it to exclusion list)
02:15:26.80 +47:49:30.1 -- not an asteroid (will add it to exclusion list)
01:39:42.90 +46:08:02.0 -- not an asteroid (will add it to exclusion list)
01:53:18.35 +50:20:13.6 -- not an asteroid (will add it to exclusion list)
01:46:55.49 +43:52:12.9 -- not an asteroid (will add it to exclusion list)
01:44:08.34 +44:31:52.3 -- not an asteroid (will add it to exclusion list)
01:46:51.96 +48:49:14.8 -- not an asteroid (will add it to exclusion list)
01:47:43.06 +41:11:40.9 -- not an asteroid (will add it to exclusion list)
01:45:06.35 +45:11:59.2 -- not an asteroid (will add it to exclusion list)
01:44:58.59 +44:13:14.9 -- not an asteroid (will add it to exclusion list)
01:41:56.40 +42:51:51.8 -- not an asteroid (will add it to exclusion list)
01:42:02.82 +48:01:53.7 -- not an asteroid (will add it to exclusion list)
01:40:49.45 +47:23:59.4 -- not an asteroid (will add it to exclusion list)
01:42:41.43 +50:53:46.8 -- not an asteroid (will add it to exclusion list)
01:43:13.44 +50:03:35.0 -- not an asteroid (will add it to exclusion list)
01:41:08.64 +47:06:56.6 -- not an asteroid (will add it to exclusion list)
01:40:00.80 +48:48:14.8 -- not an asteroid (will add it to exclusion list)
01:39:44.19 +49:12:13.0 -- not an asteroid (will add it to exclusion list)
01:42:42.91 +46:13:32.6 -- not an asteroid (will add it to exclusion list)
01:44:04.60 +41:59:53.0 -- not an asteroid (will add it to exclusion list)
01:41:33.08 +47:09:26.5 -- not an asteroid (will add it to exclusion list)
01:42:53.94 +42:39:53.6 -- not an asteroid (will add it to exclusion list)
01:41:24.25 +43:03:13.1 -- not an asteroid (will add it to exclusion list)
01:45:14.26 +50:43:02.9 -- not an asteroid (will add it to exclusion list)
01:42:19.97 +46:30:39.4 -- not an asteroid (will add it to exclusion list)
01:42:25.71 +43:04:53.1 -- not an asteroid (will add it to exclusion list)
01:43:03.08 +49:14:44.3 -- not an asteroid (will add it to exclusion list)
01:40:54.32 +45:53:13.6 -- not an asteroid (will add it to exclusion list)
01:44:36.89 +50:20:54.7 -- not an asteroid (will add it to exclusion list)
01:48:20.88 +50:22:19.2 -- not an asteroid (will add it to exclusion list)
01:42:34.81 +46:57:03.4 -- not an asteroid (will add it to exclusion list)
01:44:23.22 +50:23:38.7 -- not an asteroid (will add it to exclusion list)
01:40:18.39 +49:31:07.5 -- not an asteroid (will add it to exclusion list)
01:43:53.92 +42:44:53.9 -- not an asteroid (will add it to exclusion list)
01:41:48.43 +46:32:32.1 -- not an asteroid (will add it to exclusion list)
01:48:14.51 +41:15:36.5 -- not an asteroid (will add it to exclusion list)
01:40:50.14 +44:36:25.6 -- not an asteroid (will add it to exclusion list)
01:45:17.34 +49:27:14.3 -- not an asteroid (will add it to exclusion list)
01:46:38.45 +50:55:54.7 -- not an asteroid (will add it to exclusion list)
01:51:10.81 +50:11:41.3 -- not an asteroid (will add it to exclusion list)
01:46:26.56 +41:33:31.6 -- not an asteroid (will add it to exclusion list)
01:47:21.67 +40:56:47.3 -- not an asteroid (will add it to exclusion list)
01:44:46.48 +50:03:43.0 -- not an asteroid (will add it to exclusion list)
01:42:40.02 +48:22:31.7 -- not an asteroid (will add it to exclusion list)
01:41:58.33 +45:40:22.7 -- not an asteroid (will add it to exclusion list)
01:42:24.03 +47:31:31.3 -- not an asteroid (will add it to exclusion list)
01:42:11.68 +49:58:09.9 -- not an asteroid (will add it to exclusion list)
01:44:13.52 +50:47:28.3 -- not an asteroid (will add it to exclusion list)
01:44:21.12 +42:00:18.3 -- not an asteroid (will add it to exclusion list)
01:42:55.33 +49:06:37.4 -- not an asteroid (will add it to exclusion list)
01:47:26.71 +49:57:44.8 -- not an asteroid (will add it to exclusion list)
01:39:35.57 +49:52:19.9 -- not an asteroid (will add it to exclusion list)
01:44:35.93 +47:22:04.6 -- not an asteroid (will add it to exclusion list)
01:44:46.84 +49:40:24.1 -- not an asteroid (will add it to exclusion list)
01:44:36.47 +41:24:56.4 -- not an asteroid (will add it to exclusion list)
01:46:55.09 +41:29:32.4 -- not an asteroid (will add it to exclusion list)
01:44:38.66 +40:54:01.1 -- not an asteroid (will add it to exclusion list)
01:46:54.82 +50:17:09.6 -- not an asteroid (will add it to exclusion list)
01:47:08.56 +49:42:19.1 -- not an asteroid (will add it to exclusion list)
01:45:39.66 +50:02:45.0 -- not an asteroid (will add it to exclusion list)
01:41:51.60 +46:18:24.2 -- not an asteroid (will add it to exclusion list)
01:44:52.03 +41:57:29.3 -- not an asteroid (will add it to exclusion list)
01:47:23.38 +40:55:35.7 -- not an asteroid (will add it to exclusion list)
01:38:40.54 +48:48:07.7 -- not an asteroid (will add it to exclusion list)
01:41:00.84 +48:47:27.9 -- not an asteroid (will add it to exclusion list)
01:41:17.39 +46:27:17.1 -- not an asteroid (will add it to exclusion list)
01:38:43.41 +47:54:49.2 -- not an asteroid (will add it to exclusion list)
01:43:19.16 +41:23:19.1 -- not an asteroid (will add it to exclusion list)
01:39:08.27 +49:01:15.3 -- not an asteroid (will add it to exclusion list)
01:49:58.89 +50:47:44.2 -- not an asteroid (will add it to exclusion list)
01:44:56.88 +50:10:28.1 -- not an asteroid (will add it to exclusion list)
01:47:28.81 +41:22:25.3 -- not an asteroid (will add it to exclusion list)
01:46:54.10 +41:10:23.1 -- not an asteroid (will add it to exclusion list)
01:43:10.13 +49:54:13.0 -- not an asteroid (will add it to exclusion list)
01:40:10.55 +45:21:39.5 -- not an asteroid (will add it to exclusion list)
01:48:09.36 +50:53:40.7 -- not an asteroid (will add it to exclusion list)
01:42:50.80 +41:16:19.4 -- not an asteroid (will add it to exclusion list)
01:41:44.33 +48:56:42.4 -- not an asteroid (will add it to exclusion list)
01:49:10.98 +50:08:40.1 -- not an asteroid (will add it to exclusion list)
01:41:13.72 +49:57:03.7 -- not an asteroid (will add it to exclusion list)
01:41:37.25 +49:31:01.5 -- not an asteroid (will add it to exclusion list)
01:48:07.32 +50:18:38.5 -- not an asteroid (will add it to exclusion list)
01:43:50.29 +48:14:20.1 -- not an asteroid (will add it to exclusion list)
01:42:46.68 +41:03:48.1 -- not an asteroid (will add it to exclusion list)
01:39:03.62 +47:46:53.4 -- not an asteroid (will add it to exclusion list)
01:42:37.78 +48:32:05.4 -- not an asteroid (will add it to exclusion list)
01:40:24.35 +45:31:10.9 -- not an asteroid (will add it to exclusion list)
01:40:28.67 +50:36:02.1 -- not an asteroid (will add it to exclusion list)
01:42:31.26 +49:41:32.6 -- not an asteroid (will add it to exclusion list)
01:42:22.98 +49:10:51.3 -- not an asteroid (will add it to exclusion list)
01:47:37.68 +41:35:32.3 -- not an asteroid (will add it to exclusion list)
01:42:18.20 +47:55:50.5 -- not an asteroid (will add it to exclusion list)
01:42:15.65 +41:22:02.4 -- not an asteroid (will add it to exclusion list)
01:44:47.49 +41:00:59.5 -- not an asteroid (will add it to exclusion list)
01:44:37.14 +41:48:38.2 -- not an asteroid (will add it to exclusion list)
01:47:07.75 +49:19:04.6 -- not an asteroid (will add it to exclusion list)
01:46:38.82 +41:54:52.4 -- not an asteroid (will add it to exclusion list)
01:42:10.20 +49:43:57.1 -- not an asteroid (will add it to exclusion list)
01:41:46.28 +47:10:28.5 -- not an asteroid (will add it to exclusion list)
01:44:08.29 +50:46:10.9 -- not an asteroid (will add it to exclusion list)
01:43:05.79 +49:47:23.6 -- not an asteroid (will add it to exclusion list)
01:44:13.91 +49:20:00.7 -- not an asteroid (will add it to exclusion list)
01:47:29.28 +41:23:13.3 -- not an asteroid (will add it to exclusion list)
01:43:19.22 +44:53:54.6 -- not an asteroid (will add it to exclusion list)
01:46:37.43 +49:51:27.9 -- not an asteroid (will add it to exclusion list)
01:40:19.18 +48:29:58.1 -- not an asteroid (will add it to exclusion list)
01:45:53.39 +42:19:49.6 -- not an asteroid (will add it to exclusion list)
01:40:18.42 +50:12:24.0 -- not an asteroid (will add it to exclusion list)
01:40:39.60 +50:29:38.0 -- not an asteroid (will add it to exclusion list)
01:44:12.27 +50:35:01.8 -- not an asteroid (will add it to exclusion list)
01:47:29.12 +49:53:59.1 -- not an asteroid (will add it to exclusion list)
01:39:53.62 +46:26:13.6 -- not an asteroid (will add it to exclusion list)
01:39:54.79 +48:44:41.4 -- not an asteroid (will add it to exclusion list)
01:42:55.31 +50:35:01.2 -- not an asteroid (will add it to exclusion list)
01:39:13.66 +47:34:34.4 -- not an asteroid (will add it to exclusion list)
01:38:57.99 +48:26:44.1 -- not an asteroid (will add it to exclusion list)
01:40:15.29 +47:01:23.3 -- not an asteroid (will add it to exclusion list)
01:51:28.58 +50:40:50.0 -- not an asteroid (will add it to exclusion list)
01:41:47.73 +50:48:42.9 -- not an asteroid (will add it to exclusion list)
01:41:28.15 +50:45:37.4 -- not an asteroid (will add it to exclusion list)
01:44:09.59 +48:57:04.9 -- not an asteroid (will add it to exclusion list)
01:43:00.68 +50:24:37.4 -- not an asteroid (will add it to exclusion list)
01:40:14.97 +45:31:37.8 -- not an asteroid (will add it to exclusion list)
01:42:57.72 +42:19:18.6 -- not an asteroid (will add it to exclusion list)
01:42:50.32 +45:52:17.2 -- not an asteroid (will add it to exclusion list)
01:43:37.77 +47:25:45.4 -- not an asteroid (will add it to exclusion list)
01:41:30.75 +43:52:17.3 -- not an asteroid (will add it to exclusion list)
01:47:08.66 +40:59:47.9 -- not an asteroid (will add it to exclusion list)
01:42:29.49 +47:16:49.1 -- not an asteroid (will add it to exclusion list)
01:42:15.76 +41:27:52.2 -- not an asteroid (will add it to exclusion list)
01:42:51.08 +43:06:44.4 -- not an asteroid (will add it to exclusion list)
01:43:36.69 +41:13:27.0 -- not an asteroid (will add it to exclusion list)
01:44:10.00 +41:26:56.9 -- not an asteroid (will add it to exclusion list)
01:42:55.50 +41:25:28.6 -- not an asteroid (will add it to exclusion list)
01:46:27.43 +50:15:31.0 -- not an asteroid (will add it to exclusion list)
01:46:43.96 +41:33:49.0 -- not an asteroid (will add it to exclusion list)
01:40:58.36 +44:53:38.1 -- not an asteroid (will add it to exclusion list)
01:43:42.36 +48:22:35.3 -- not an asteroid (will add it to exclusion list)
01:40:07.54 +47:00:48.3 -- not an asteroid (will add it to exclusion list)
01:37:53.81 +49:31:02.6 -- not an asteroid (will add it to exclusion list)
01:41:03.82 +44:44:46.8 -- not an asteroid (will add it to exclusion list)
01:39:23.28 +50:19:09.9 -- not an asteroid (will add it to exclusion list)
01:48:08.64 +49:34:01.7 -- not an asteroid (will add it to exclusion list)
01:44:47.42 +50:21:23.8 -- not an asteroid (will add it to exclusion list)
01:45:59.06 +40:53:19.0 -- not an asteroid (will add it to exclusion list)
01:40:05.34 +49:36:51.7 -- not an asteroid (will add it to exclusion list)
01:44:22.23 +45:26:14.8 -- not an asteroid (will add it to exclusion list)
01:41:37.79 +45:33:04.7 -- not an asteroid (will add it to exclusion list)
01:43:29.86 +49:41:03.1 -- not an asteroid (will add it to exclusion list)
01:44:31.98 +50:40:49.8 -- not an asteroid (will add it to exclusion list)
01:44:40.03 +41:26:50.8 -- not an asteroid (will add it to exclusion list)
01:40:10.42 +50:40:29.6 -- not an asteroid (will add it to exclusion list)
01:38:44.76 +49:37:45.6 -- not an asteroid (will add it to exclusion list)
01:45:52.22 +48:57:57.0 -- not an asteroid (will add it to exclusion list)
01:43:32.43 +50:24:35.3 -- not an asteroid (will add it to exclusion list)
01:37:31.29 +50:24:10.9 -- not an asteroid (will add it to exclusion list)
01:45:33.11 +50:14:55.2 -- not an asteroid (will add it to exclusion list)
01:46:42.32 +50:10:12.3 -- not an asteroid (will add it to exclusion list)
01:44:12.08 +42:09:50.1 -- not an asteroid (will add it to exclusion list)
01:42:46.71 +48:02:54.1 -- not an asteroid (will add it to exclusion list)
01:47:07.49 +41:16:33.6 -- not an asteroid (will add it to exclusion list)
01:45:53.14 +49:31:40.4 -- not an asteroid (will add it to exclusion list)
01:48:01.76 +49:58:50.0 -- not an asteroid (will add it to exclusion list)
01:41:34.03 +47:35:43.1 -- not an asteroid (will add it to exclusion list)
01:39:11.47 +49:22:07.7 -- not an asteroid (will add it to exclusion list)
01:46:23.83 +50:05:58.0 -- not an asteroid (will add it to exclusion list)
01:41:39.17 +46:45:57.0 -- not an asteroid (will add it to exclusion list)
01:38:16.29 +49:36:44.0 -- not an asteroid (will add it to exclusion list)
01:39:11.32 +47:26:23.9 -- not an asteroid (will add it to exclusion list)
01:41:39.83 +43:15:07.9 -- not an asteroid (will add it to exclusion list)
01:41:47.04 +42:49:16.7 -- not an asteroid (will add it to exclusion list)
01:43:57.46 +44:22:08.2 -- not an asteroid (will add it to exclusion list)
01:40:01.06 +46:44:49.1 -- not an asteroid (will add it to exclusion list)
01:45:23.80 +41:52:27.9 -- not an asteroid (will add it to exclusion list)
01:47:39.04 +41:09:46.3 -- not an asteroid (will add it to exclusion list)
01:42:35.62 +43:19:12.3 -- not an asteroid (will add it to exclusion list)
01:41:34.81 +50:04:10.2 -- not an asteroid (will add it to exclusion list)
01:44:47.62 +47:52:24.7 -- not an asteroid (will add it to exclusion list)
01:45:47.96 +50:04:49.7 -- not an asteroid (will add it to exclusion list)
01:45:14.42 +49:04:08.3 -- not an asteroid (will add it to exclusion list)
01:46:04.17 +42:10:40.0 -- not an asteroid (will add it to exclusion list)
01:40:10.03 +47:23:35.8 -- not an asteroid (will add it to exclusion list)
01:45:15.59 +49:25:52.2 -- not an asteroid (will add it to exclusion list)
01:43:55.65 +43:11:05.6 -- not an asteroid (will add it to exclusion list)
01:51:13.71 +50:00:48.0 -- not an asteroid (will add it to exclusion list)
01:43:08.01 +41:05:22.5 -- not an asteroid (will add it to exclusion list)
01:40:26.75 +50:42:36.7 -- not an asteroid (will add it to exclusion list)
01:38:52.27 +49:43:52.5 -- not an asteroid (will add it to exclusion list)
01:41:22.02 +43:22:47.8 -- not an asteroid (will add it to exclusion list)
01:41:51.87 +44:47:41.4 -- not an asteroid (will add it to exclusion list)
01:45:00.36 +50:35:25.7 -- not an asteroid (will add it to exclusion list)
01:41:52.74 +48:30:11.1 -- not an asteroid (will add it to exclusion list)
01:41:09.12 +50:32:09.1 -- not an asteroid (will add it to exclusion list)
01:45:13.52 +50:03:38.4 -- not an asteroid (will add it to exclusion list)
01:41:16.39 +50:02:34.2 -- not an asteroid (will add it to exclusion list)
01:45:44.25 +48:18:31.2 -- not an asteroid (will add it to exclusion list)
01:43:03.73 +50:33:40.0 -- not an asteroid (will add it to exclusion list)
01:46:28.14 +49:35:08.9 -- not an asteroid (will add it to exclusion list)
01:45:55.88 +50:44:39.8 -- not an asteroid (will add it to exclusion list)
01:42:35.85 +41:06:58.6 -- not an asteroid (will add it to exclusion list)
01:50:37.60 +50:34:55.7 -- not an asteroid (will add it to exclusion list)
01:39:43.63 +46:42:23.2 -- not an asteroid (will add it to exclusion list)
01:41:31.88 +43:16:12.5 -- not an asteroid (will add it to exclusion list)
01:41:29.77 +42:45:16.0 -- not an asteroid (will add it to exclusion list)
01:41:46.39 +44:21:09.3 -- not an asteroid (will add it to exclusion list)
01:43:12.02 +50:32:39.7 -- not an asteroid (will add it to exclusion list)
01:43:58.52 +47:40:24.8 -- not an asteroid (will add it to exclusion list)
01:46:25.78 +41:40:10.5 -- not an asteroid (will add it to exclusion list)
01:40:20.90 +50:28:37.1 -- not an asteroid (will add it to exclusion list)
01:44:34.81 +42:55:59.7 -- not an asteroid (will add it to exclusion list)
01:46:00.65 +50:03:46.1 -- not an asteroid (will add it to exclusion list)
01:41:56.25 +42:44:53.5 -- not an asteroid (will add it to exclusion list)
02:22:26.91 +42:18:07.3 -- not an asteroid (will add it to exclusion list)
01:42:40.09 +41:50:36.9 -- not an asteroid (will add it to exclusion list)
01:44:48.28 +40:57:58.0 -- not an asteroid (will add it to exclusion list)
01:38:10.39 +50:22:34.6 -- not an asteroid (will add it to exclusion list)
01:47:13.39 +50:08:57.4 -- not an asteroid (will add it to exclusion list)
01:42:02.91 +41:38:42.5 -- not an asteroid (will add it to exclusion list)
01:41:20.24 +49:23:44.2 -- not an asteroid (will add it to exclusion list)
01:41:40.64 +50:38:38.2 -- not an asteroid (will add it to exclusion list)
01:46:40.73 +49:57:41.8 -- not an asteroid (will add it to exclusion list)
01:56:48.56 +43:10:17.5 -- not an asteroid (will add it to exclusion list)
01:40:26.67 +49:25:27.3 -- not an asteroid (will add it to exclusion list)
01:42:45.77 +42:01:56.6 -- not an asteroid (will add it to exclusion list)
01:41:05.23 +44:36:05.5 -- not an asteroid (will add it to exclusion list)
01:48:38.44 +50:20:15.2 -- not an asteroid (will add it to exclusion list)
01:44:30.20 +50:39:18.1 -- not an asteroid (will add it to exclusion list)
01:45:34.46 +49:47:07.4 -- not an asteroid (will add it to exclusion list)
01:42:44.88 +50:12:26.3 -- not an asteroid (will add it to exclusion list)
01:41:52.77 +44:11:18.7 -- not an asteroid (will add it to exclusion list)
01:48:45.20 +50:33:06.6 -- not an asteroid (will add it to exclusion list)
01:54:13.09 +50:55:58.7 -- not an asteroid (will add it to exclusion list)
01:42:51.48 +50:52:29.6 -- not an asteroid (will add it to exclusion list)
02:18:18.35 +49:53:11.9 -- not an asteroid (will add it to exclusion list)
01:46:38.46 +41:34:18.3 -- not an asteroid (will add it to exclusion list)
01:40:33.18 +49:47:52.3 -- not an asteroid (will add it to exclusion list)
01:39:04.13 +49:43:21.1 -- not an asteroid (will add it to exclusion list)
01:45:11.61 +49:46:13.1 -- not an asteroid (will add it to exclusion list)
01:45:19.00 +42:29:43.3 -- not an asteroid (will add it to exclusion list)
01:42:53.36 +41:42:06.2 -- not an asteroid (will add it to exclusion list)
01:42:24.83 +43:21:44.5 -- not an asteroid (will add it to exclusion list)
01:39:29.18 +50:16:33.7 -- not an asteroid (will add it to exclusion list)
01:53:01.77 +50:59:18.7 -- not an asteroid (will add it to exclusion list)
01:41:41.33 +49:43:08.2 -- not an asteroid (will add it to exclusion list)
01:43:37.79 +43:49:53.3 -- not an asteroid (will add it to exclusion list)
01:43:27.48 +50:28:06.0 -- not an asteroid (will add it to exclusion list)
01:43:11.97 +44:52:32.4 -- not an asteroid (will add it to exclusion list)
01:46:10.95 +49:00:54.1 -- not an asteroid (will add it to exclusion list)
01:38:20.74 +50:37:24.7 -- not an asteroid (will add it to exclusion list)
01:46:28.51 +49:52:23.4 -- not an asteroid (will add it to exclusion list)
01:41:32.61 +49:02:41.5 -- not an asteroid (will add it to exclusion list)
01:44:12.76 +41:15:28.4 -- not an asteroid (will add it to exclusion list)
01:42:25.29 +41:30:33.2 -- not an asteroid (will add it to exclusion list)
01:41:32.23 +45:53:25.1 -- not an asteroid (will add it to exclusion list)
01:45:22.30 +49:57:25.0 -- not an asteroid (will add it to exclusion list)
01:39:38.57 +48:18:37.7 -- not an asteroid (will add it to exclusion list)
01:49:03.79 +41:05:49.8 -- not an asteroid (will add it to exclusion list)
01:40:20.89 +48:05:07.4 -- not an asteroid (will add it to exclusion list)
01:52:01.75 +50:43:20.4 -- not an asteroid (will add it to exclusion list)
01:47:27.45 +49:45:10.3 -- not an asteroid (will add it to exclusion list)
01:43:02.95 +50:49:28.9 -- not an asteroid (will add it to exclusion list)
01:47:18.94 +49:50:41.9 -- not an asteroid (will add it to exclusion list)
01:42:20.08 +50:49:16.0 -- not an asteroid (will add it to exclusion list)
01:43:23.89 +42:07:14.2 -- not an asteroid (will add it to exclusion list)
01:38:43.91 +48:34:01.6 -- not an asteroid (will add it to exclusion list)
01:39:18.03 +48:11:10.5 -- not an asteroid (will add it to exclusion list)
01:43:18.98 +50:21:32.1 -- not an asteroid (will add it to exclusion list)
01:44:27.99 +50:36:09.1 -- not an asteroid (will add it to exclusion list)
01:45:47.48 +40:55:31.0 -- not an asteroid (will add it to exclusion list)
01:41:34.51 +50:12:58.6 -- not an asteroid (will add it to exclusion list)
01:40:19.08 +50:48:57.1 -- not an asteroid (will add it to exclusion list)
01:43:41.87 +40:50:33.1 -- not an asteroid (will add it to exclusion list)
01:42:06.04 +49:51:07.1 -- not an asteroid (will add it to exclusion list)
01:48:01.18 +40:58:04.6 -- not an asteroid (will add it to exclusion list)
01:37:53.96 +49:36:12.5 -- not an asteroid (will add it to exclusion list)
01:39:22.89 +49:33:38.1 -- not an asteroid (will add it to exclusion list)
01:41:59.00 +49:23:43.8 -- not an asteroid (will add it to exclusion list)
01:44:27.15 +41:10:32.2 -- not an asteroid (will add it to exclusion list)
01:38:20.35 +50:37:01.3 -- not an asteroid (will add it to exclusion list)
01:40:13.36 +49:51:56.8 -- not an asteroid (will add it to exclusion list)
01:43:17.75 +50:48:53.9 -- not an asteroid (will add it to exclusion list)
01:39:15.98 +49:06:39.2 -- not an asteroid (will add it to exclusion list)
01:40:30.40 +47:19:17.1 -- not an asteroid (will add it to exclusion list)
01:44:46.17 +41:07:25.0 -- not an asteroid (will add it to exclusion list)
01:45:58.19 +41:00:40.6 -- not an asteroid (will add it to exclusion list)
01:44:32.18 +50:29:57.3 -- not an asteroid (will add it to exclusion list)
01:45:07.56 +40:53:48.6 -- not an asteroid (will add it to exclusion list)
01:39:12.53 +48:41:45.9 -- not an asteroid (will add it to exclusion list)
01:42:07.84 +50:03:45.1 -- not an asteroid (will add it to exclusion list)
01:45:19.09 +42:16:51.5 -- not an asteroid (will add it to exclusion list)
01:38:11.35 +50:28:56.2 -- not an asteroid (will add it to exclusion list)
01:41:52.76 +43:11:19.5 -- not an asteroid (will add it to exclusion list)
01:39:50.55 +46:04:05.1 -- not an asteroid (will add it to exclusion list)
01:41:53.55 +49:30:18.0 -- not an asteroid (will add it to exclusion list)
01:38:41.14 +48:13:18.4 -- not an asteroid (will add it to exclusion list)
01:39:14.44 +50:19:46.5 -- not an asteroid (will add it to exclusion list)
01:43:35.00 +50:17:09.0 -- not an asteroid (will add it to exclusion list)
01:45:14.37 +40:53:42.7 -- not an asteroid (will add it to exclusion list)
01:46:24.88 +50:22:00.8 -- not an asteroid (will add it to exclusion list)
01:37:14.74 +50:41:50.2 -- not an asteroid (will add it to exclusion list)
01:41:13.93 +50:12:17.6 -- not an asteroid (will add it to exclusion list)
01:43:48.98 +42:02:42.4 -- not an asteroid (will add it to exclusion list)
01:40:06.33 +46:27:55.9 -- not an asteroid (will add it to exclusion list)
01:43:10.86 +49:20:43.3 -- not an asteroid (will add it to exclusion list)
01:41:40.69 +49:13:48.9 -- not an asteroid (will add it to exclusion list)
01:42:00.01 +42:10:17.7 -- not an asteroid (will add it to exclusion list)
01:45:19.84 +41:07:56.5 -- not an asteroid (will add it to exclusion list)
01:44:56.77 +48:16:07.7 -- not an asteroid (will add it to exclusion list)
01:46:04.56 +40:54:34.9 -- not an asteroid (will add it to exclusion list)
01:39:21.30 +49:18:05.4 -- not an asteroid (will add it to exclusion list)
01:44:04.71 +50:31:10.7 -- not an asteroid (will add it to exclusion list)
01:40:47.42 +49:33:53.7 -- not an asteroid (will add it to exclusion list)
01:38:12.28 +49:40:34.7 -- not an asteroid (will add it to exclusion list)
01:41:31.22 +50:15:16.3 -- not an asteroid (will add it to exclusion list)
01:47:32.15 +41:04:11.7 -- not an asteroid (will add it to exclusion list)
01:43:43.30 +41:17:08.3 -- not an asteroid (will add it to exclusion list)
01:42:51.60 +41:39:26.6 -- not an asteroid (will add it to exclusion list)
01:43:01.94 +43:18:08.2 -- not an asteroid (will add it to exclusion list)
01:46:43.80 +41:23:12.3 -- not an asteroid (will add it to exclusion list)
01:42:41.60 +41:01:11.6 -- not an asteroid (will add it to exclusion list)
01:45:17.70 +41:05:12.1 -- not an asteroid (will add it to exclusion list)
01:45:18.13 +42:02:14.0 -- not an asteroid (will add it to exclusion list)
01:44:14.83 +49:40:51.5 -- not an asteroid (will add it to exclusion list)
01:44:33.13 +41:50:18.8 -- not an asteroid (will add it to exclusion list)
01:41:35.59 +43:18:35.1 -- not an asteroid (will add it to exclusion list)
02:56:41.72 +50:33:24.5 -- not an asteroid (will add it to exclusion list)
01:46:00.02 +42:35:07.2 -- not an asteroid (will add it to exclusion list)
02:23:03.21 +48:12:01.7 -- not an asteroid (will add it to exclusion list)
01:42:11.71 +43:36:15.4 -- not an asteroid (will add it to exclusion list)
02:36:24.20 +44:54:58.7 -- not an asteroid (will add it to exclusion list)
02:48:15.68 +44:37:04.6 -- not an asteroid (will add it to exclusion list)
02:18:55.22 +45:28:22.0 -- not an asteroid (will add it to exclusion list)
01:46:16.24 +41:33:49.5 -- not an asteroid (will add it to exclusion list)
02:59:56.11 +42:37:15.3 -- not an asteroid (will add it to exclusion list)
02:28:25.37 +45:36:03.5 -- not an asteroid (will add it to exclusion list)
01:45:47.56 +44:49:48.8 -- not an asteroid (will add it to exclusion list)
01:40:54.69 +48:17:03.5 -- not an asteroid (will add it to exclusion list)
02:33:48.96 +45:12:54.0 -- not an asteroid (will add it to exclusion list)
01:44:34.37 +40:54:48.1 -- not an asteroid (will add it to exclusion list)
02:32:11.23 +49:54:37.5 -- not an asteroid (will add it to exclusion list)
02:33:46.26 +48:29:08.9 -- not an asteroid (will add it to exclusion list)
01:43:52.46 +48:56:35.1 -- not an asteroid (will add it to exclusion list)
01:41:47.35 +42:23:36.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
01:37:14.74 +50:41:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:31.29 +50:24:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:49.92 +50:22:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:53.07 +50:36:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:53.81 +49:31:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:53.96 +49:36:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:04.85 +49:25:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:10.39 +50:22:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:11.35 +50:28:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:12.28 +49:40:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:16.29 +49:36:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:20.35 +50:37:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:20.74 +50:37:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:22.85 +49:17:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:40.54 +48:48:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:41.14 +48:13:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:43.41 +47:54:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:43.91 +48:34:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:44.23 +48:52:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:44.76 +49:37:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:52.27 +49:43:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:38:57.99 +48:26:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:03.62 +47:46:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:04.13 +49:43:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:05.41 +49:30:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:08.27 +49:01:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:11.32 +47:26:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:11.47 +49:22:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:12.53 +48:41:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:13.66 +47:34:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:14.44 +50:19:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:15.98 +49:06:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:18.03 +48:11:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:19.25 +49:36:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:21.30 +49:18:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:22.89 +49:33:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:23.28 +50:19:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:29.18 +50:16:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:31.97 +50:29:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:35.57 +49:52:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:38.57 +48:18:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:39.94 +47:00:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:41.54 +49:00:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:42.90 +46:08:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:43.63 +46:42:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:44.19 +49:12:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:48.75 +47:33:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:50.16 +50:35:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:50.55 +46:04:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:53.62 +46:26:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:54.79 +48:44:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:39:55.75 +46:38:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:00.80 +48:48:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:01.06 +46:44:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:05.34 +49:36:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:05.55 +50:08:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:06.33 +46:27:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:07.54 +47:00:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:10.03 +47:23:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:10.42 +50:40:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:10.55 +45:21:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:13.36 +49:51:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:14.97 +45:31:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:15.25 +46:10:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:15.29 +47:01:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:18.39 +49:31:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:18.42 +50:12:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:19.08 +50:48:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:19.18 +48:29:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:20.89 +48:05:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:20.90 +50:28:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:24.35 +45:31:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:24.74 +49:45:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:26.67 +49:25:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:26.75 +50:42:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:28.67 +50:36:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:30.40 +47:19:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:33.18 +49:47:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:36.95 +50:47:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:39.39 +45:07:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:39.60 +50:29:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:40.90 +50:16:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:43.59 +50:37:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:47.42 +49:33:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:49.45 +47:23:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:50.14 +44:36:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:52.67 +50:18:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:54.32 +45:53:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:54.69 +48:17:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:40:58.36 +44:53:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:00.84 +48:47:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:03.82 +44:44:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:05.23 +44:36:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:08.64 +47:06:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:09.12 +50:32:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:13.72 +49:57:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:13.93 +50:12:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:14.46 +46:52:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:16.39 +50:02:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:17.39 +46:27:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:20.14 +44:02:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:20.24 +49:23:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:22.02 +43:22:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:24.25 +43:03:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:24.74 +44:25:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:28.15 +50:45:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:29.77 +42:45:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:30.75 +43:52:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:31.22 +50:15:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:31.88 +43:16:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:32.23 +45:53:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:32.61 +49:02:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:33.08 +47:09:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:34.03 +47:35:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:34.51 +50:12:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:34.81 +50:04:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:35.59 +43:18:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:37.25 +49:31:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:37.79 +45:33:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:39.06 +48:45:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:39.17 +46:45:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:39.83 +43:15:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:40.64 +50:38:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:40.69 +49:13:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:41.33 +49:43:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:44.33 +48:56:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:46.28 +47:10:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:46.39 +44:21:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:47.04 +42:49:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:47.35 +42:23:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:47.73 +50:48:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:48.43 +46:32:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:50.30 +48:40:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:50.50 +46:01:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:50.52 +48:08:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:51.60 +46:18:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:51.87 +44:47:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:52.74 +48:30:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:52.76 +43:11:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:52.77 +44:11:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:53.55 +49:30:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:56.25 +42:44:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:56.40 +42:51:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:58.33 +45:40:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:41:59.00 +49:23:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:00.01 +42:10:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:02.82 +48:01:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:02.91 +41:38:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:04.22 +48:01:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:06.04 +49:51:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:07.84 +50:03:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:08.85 +48:05:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:10.20 +49:43:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:11.64 +48:17:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:11.68 +49:58:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:11.71 +43:36:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:12.31 +48:06:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:15.65 +41:22:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:15.76 +41:27:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:16.45 +46:55:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:16.72 +42:18:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:18.20 +47:55:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:19.97 +46:30:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:20.08 +50:49:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:22.98 +49:10:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:24.03 +47:31:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:24.83 +43:21:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:25.29 +41:30:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:25.71 +43:04:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:29.49 +47:16:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:31.26 +49:41:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:34.81 +46:57:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:35.62 +43:19:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:35.85 +41:06:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:36.23 +48:56:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:37.78 +48:32:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:40.02 +48:22:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:40.09 +41:50:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:40.68 +42:38:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:41.43 +50:53:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:41.60 +41:01:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:42.91 +46:13:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:44.88 +50:12:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:45.77 +42:01:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:46.68 +41:03:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:46.71 +48:02:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:50.32 +45:52:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:50.80 +41:16:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:50.83 +43:56:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:51.08 +43:06:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:51.28 +47:36:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:51.48 +50:52:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:51.60 +41:39:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:53.36 +41:42:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:53.39 +43:50:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:53.94 +42:39:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:55.31 +50:35:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:55.33 +49:06:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:55.50 +41:25:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:42:57.72 +42:19:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:00.68 +50:24:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:01.94 +43:18:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:02.95 +50:49:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:03.01 +45:47:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:03.08 +49:14:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:03.73 +50:33:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:05.79 +49:47:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:08.01 +41:05:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:10.13 +49:54:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:10.86 +49:20:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:11.97 +44:52:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:12.02 +50:32:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:13.44 +50:03:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:14.67 +42:13:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:16.49 +45:50:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:17.24 +44:50:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:17.75 +50:48:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:18.98 +50:21:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:19.16 +41:23:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:19.22 +44:53:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:23.89 +42:07:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:27.48 +50:28:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:28.37 +42:52:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:29.86 +49:41:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:31.36 +49:36:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:32.43 +50:24:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:35.00 +50:17:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:36.69 +41:13:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:37.26 +44:07:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:37.77 +47:25:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:37.79 +43:49:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:41.87 +40:50:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:42.36 +48:22:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:42.62 +43:18:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:43.30 +41:17:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:45.28 +43:49:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:48.98 +42:02:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:50.29 +48:14:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:52.46 +48:56:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:53.92 +42:44:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:55.65 +43:11:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:57.46 +44:22:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:43:58.52 +47:40:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:04.60 +41:59:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:04.71 +50:31:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:07.77 +43:59:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:08.29 +50:46:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:08.34 +44:31:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:09.59 +48:57:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:10.00 +41:26:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:10.11 +45:00:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:12.08 +42:09:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:12.27 +50:35:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:12.76 +41:15:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:13.52 +50:47:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:13.91 +49:20:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:14.23 +47:19:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:14.83 +49:40:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:15.38 +42:56:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:15.75 +46:40:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:20.56 +44:14:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:21.07 +50:27:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:21.12 +42:00:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:22.23 +45:26:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:22.30 +46:13:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:23.22 +50:23:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:23.44 +47:33:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:24.54 +43:41:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:25.79 +43:43:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:27.15 +41:10:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:27.99 +50:36:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:28.02 +45:05:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:30.20 +50:39:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:31.98 +50:40:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:32.18 +50:29:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:33.13 +41:50:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:34.37 +40:54:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:34.81 +42:55:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:35.93 +47:22:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:36.44 +41:10:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:36.47 +41:24:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:36.89 +50:20:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:37.14 +41:48:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:38.66 +40:54:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:40.03 +41:26:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:45.60 +43:15:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:46.17 +41:07:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:46.48 +50:03:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:46.84 +49:40:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:47.42 +50:21:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:47.49 +41:00:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:47.62 +47:52:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:48.28 +40:57:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:48.52 +43:53:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:48.85 +41:56:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:49.63 +49:57:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:52.03 +41:57:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:56.77 +48:16:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:56.88 +50:10:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:44:58.59 +44:13:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:00.36 +50:35:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:06.35 +45:11:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:07.56 +40:53:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:11.31 +49:00:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:11.61 +49:46:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:13.52 +50:03:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:14.26 +50:43:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:14.37 +40:53:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:14.42 +49:04:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:15.59 +49:25:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:17.34 +49:27:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:17.70 +41:05:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:18.13 +42:02:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:19.00 +42:29:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:19.09 +42:16:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:19.84 +41:07:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:22.30 +49:57:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:23.80 +41:52:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:27.42 +50:12:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:29.89 +43:20:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:30.58 +49:51:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:30.78 +41:03:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:33.11 +50:14:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:34.46 +49:47:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:39.66 +50:02:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:44.25 +48:18:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:47.48 +40:55:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:47.56 +44:49:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:47.96 +50:04:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:48.81 +44:58:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:52.22 +48:57:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:53.14 +49:31:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:53.39 +42:19:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:55.88 +50:44:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:57.46 +49:08:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:58.19 +41:00:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:45:59.06 +40:53:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:00.02 +42:35:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:00.65 +50:03:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:04.17 +42:10:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:04.56 +40:54:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:07.54 +48:37:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:08.35 +42:12:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:10.89 +50:35:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:10.95 +49:00:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:14.29 +42:48:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:16.24 +41:33:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:17.19 +45:40:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:23.83 +50:05:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:24.88 +50:22:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:25.78 +41:40:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:26.56 +41:33:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:27.43 +50:15:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:28.14 +49:35:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:28.51 +49:52:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:33.45 +43:54:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:37.43 +49:51:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.45 +50:55:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.46 +41:34:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:38.82 +41:54:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:40.73 +49:57:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:42.32 +50:10:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:43.80 +41:23:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:43.96 +41:33:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:51.96 +48:49:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:54.10 +41:10:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:54.82 +50:17:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:55.09 +41:29:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:55.49 +43:52:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:46:56.64 +43:04:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:04.56 +47:43:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:07.49 +41:16:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:07.75 +49:19:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:08.56 +49:42:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:08.59 +48:09:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:08.66 +40:59:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:12.50 +42:46:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:13.39 +50:08:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:18.94 +49:50:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:21.67 +40:56:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:23.38 +40:55:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:23.85 +49:04:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:26.71 +49:57:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:27.45 +49:45:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:28.81 +41:22:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:29.12 +49:53:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:29.28 +41:23:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:31.65 +41:51:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:32.15 +41:04:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:37.68 +41:35:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:39.04 +41:09:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:43.06 +41:11:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:47:43.77 +41:03:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:01.18 +40:58:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:01.76 +49:58:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:07.32 +50:18:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:08.64 +49:34:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:09.36 +50:53:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:14.51 +41:15:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:15.53 +41:20:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:16.75 +42:23:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:18.99 +49:06:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:20.88 +50:22:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:29.42 +41:01:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:38.44 +50:20:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:45.20 +50:33:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:48:59.66 +48:12:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:01.06 +41:15:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:03.79 +41:05:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:10.98 +50:08:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:28.57 +41:36:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:44.56 +49:53:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:50.70 +49:46:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:57.88 +49:25:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:49:58.89 +50:47:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:37.60 +50:34:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:50:45.68 +49:47:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:10.81 +50:11:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:11.71 +41:34:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:13.32 +50:27:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:13.71 +50:00:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:14.68 +50:50:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:15.90 +49:44:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:28.58 +50:40:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:01.75 +50:43:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:52:40.28 +41:27:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:01.77 +50:59:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:53:18.35 +50:20:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:54:13.09 +50:55:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:56:48.56 +43:10:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:59:16.34 +50:55:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:11:02.76 +48:56:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:13:12.76 +49:57:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:15:26.80 +47:49:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:18.35 +49:53:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:18:55.22 +45:28:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:22:26.91 +42:18:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:23:03.21 +48:12:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:25:53.93 +46:25:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:28:25.37 +45:36:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:11.23 +49:54:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:46.05 +46:29:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:32:53.71 +48:20:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:46.26 +48:29:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:33:48.96 +45:12:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:35:51.44 +49:18:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:36:24.20 +44:54:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:38:12.61 +47:05:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:48:15.68 +44:37:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:52:22.70 +48:39:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:41.72 +50:33:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:56.11 +42:37:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
01:37:14.74 +50:41:50.2 -- not a known variable star
01:37:31.29 +50:24:10.9 -- not a known variable star
01:37:49.92 +50:22:14.3 -- not a known variable star
01:37:53.07 +50:36:24.1 -- not a known variable star
01:37:53.81 +49:31:02.6 -- not a known variable star
01:37:53.96 +49:36:12.5 -- not a known variable star
01:38:04.85 +49:25:59.4 -- not a known variable star
01:38:10.39 +50:22:34.6 -- not a known variable star
01:38:11.35 +50:28:56.2 -- not a known variable star
01:38:12.28 +49:40:34.7 -- not a known variable star
01:38:16.29 +49:36:44.0 -- a known variable star
01:38:20.35 +50:37:01.3 -- not a known variable star
01:38:20.74 +50:37:24.7 -- not a known variable star
01:38:22.85 +49:17:20.3 -- not a known variable star
01:38:40.54 +48:48:07.7 -- not a known variable star
01:38:41.14 +48:13:18.4 -- not a known variable star
01:38:43.41 +47:54:49.2 -- not a known variable star
01:38:43.91 +48:34:01.6 -- not a known variable star
01:38:44.23 +48:52:47.3 -- not a known variable star
01:38:44.76 +49:37:45.6 -- not a known variable star
01:38:52.27 +49:43:52.5 -- a known variable star
01:38:57.99 +48:26:44.1 -- not a known variable star
01:39:03.62 +47:46:53.4 -- a known variable star
01:39:04.13 +49:43:21.1 -- not a known variable star
01:39:05.41 +49:30:51.1 -- not a known variable star
01:39:08.27 +49:01:15.3 -- not a known variable star
01:39:11.32 +47:26:23.9 -- not a known variable star
01:39:11.47 +49:22:07.7 -- not a known variable star
01:39:12.53 +48:41:45.9 -- not a known variable star
01:39:13.66 +47:34:34.4 -- a known variable star
01:39:14.44 +50:19:46.5 -- not a known variable star
01:39:15.98 +49:06:39.2 -- not a known variable star
01:39:18.03 +48:11:10.5 -- not a known variable star
01:39:19.25 +49:36:17.6 -- not a known variable star
01:39:21.30 +49:18:05.4 -- not a known variable star
01:39:22.89 +49:33:38.1 -- not a known variable star
01:39:23.28 +50:19:09.9 -- not a known variable star
01:39:29.18 +50:16:33.7 -- not a known variable star
01:39:31.97 +50:29:42.3 -- a known variable star
01:39:35.57 +49:52:19.9 -- not a known variable star
01:39:38.57 +48:18:37.7 -- not a known variable star
01:39:39.94 +47:00:40.7 -- not a known variable star
01:39:41.54 +49:00:13.9 -- not a known variable star
01:39:42.90 +46:08:02.0 -- not a known variable star
01:39:43.63 +46:42:23.2 -- not a known variable star
01:39:44.19 +49:12:13.0 -- not a known variable star
01:39:48.75 +47:33:06.6 -- not a known variable star
01:39:50.16 +50:35:55.4 -- not a known variable star
01:39:50.55 +46:04:05.1 -- not a known variable star
01:39:53.62 +46:26:13.6 -- not a known variable star
01:39:54.79 +48:44:41.4 -- not a known variable star
01:39:55.75 +46:38:07.0 -- not a known variable star
01:40:00.80 +48:48:14.8 -- not a known variable star
01:40:01.06 +46:44:49.1 -- not a known variable star
01:40:05.34 +49:36:51.7 -- not a known variable star
01:40:05.55 +50:08:11.8 -- not a known variable star
01:40:06.33 +46:27:55.9 -- not a known variable star
01:40:07.54 +47:00:48.3 -- not a known variable star
01:40:10.03 +47:23:35.8 -- not a known variable star
01:40:10.42 +50:40:29.6 -- not a known variable star
01:40:10.55 +45:21:39.5 -- not a known variable star
01:40:13.36 +49:51:56.8 -- not a known variable star
01:40:14.97 +45:31:37.8 -- a known variable star
01:40:15.25 +46:10:41.1 -- not a known variable star
01:40:15.29 +47:01:23.3 -- not a known variable star
01:40:18.39 +49:31:07.5 -- not a known variable star
01:40:18.42 +50:12:24.0 -- not a known variable star
01:40:19.08 +50:48:57.1 -- not a known variable star
01:40:19.18 +48:29:58.1 -- not a known variable star
01:40:20.89 +48:05:07.4 -- a known variable star
01:40:20.90 +50:28:37.1 -- not a known variable star
01:40:24.35 +45:31:10.9 -- not a known variable star
01:40:24.74 +49:45:59.4 -- not a known variable star
01:40:26.67 +49:25:27.3 -- not a known variable star
01:40:26.75 +50:42:36.7 -- not a known variable star
01:40:28.67 +50:36:02.1 -- not a known variable star
01:40:30.40 +47:19:17.1 -- not a known variable star
01:40:33.18 +49:47:52.3 -- not a known variable star
01:40:36.95 +50:47:45.7 -- not a known variable star
01:40:39.39 +45:07:34.2 -- not a known variable star
01:40:39.60 +50:29:38.0 -- not a known variable star
01:40:40.90 +50:16:46.3 -- not a known variable star
01:40:43.59 +50:37:31.8 -- not a known variable star
01:40:47.42 +49:33:53.7 -- a known variable star
01:40:49.45 +47:23:59.4 -- not a known variable star
01:40:50.14 +44:36:25.6 -- not a known variable star
01:40:52.67 +50:18:02.5 -- not a known variable star
01:40:54.32 +45:53:13.6 -- not a known variable star
01:40:54.69 +48:17:03.5 -- not a known variable star
01:40:58.36 +44:53:38.1 -- not a known variable star
01:41:00.84 +48:47:27.9 -- not a known variable star
01:41:03.82 +44:44:46.8 -- not a known variable star
01:41:05.23 +44:36:05.5 -- not a known variable star
01:41:08.64 +47:06:56.6 -- not a known variable star
01:41:09.12 +50:32:09.1 -- not a known variable star
01:41:13.72 +49:57:03.7 -- not a known variable star
01:41:13.93 +50:12:17.6 -- not a known variable star
01:41:14.46 +46:52:03.6 -- not a known variable star
01:41:16.39 +50:02:34.2 -- not a known variable star
01:41:17.39 +46:27:17.1 -- not a known variable star
01:41:20.14 +44:02:27.9 -- not a known variable star
01:41:20.24 +49:23:44.2 -- not a known variable star
01:41:22.02 +43:22:47.8 -- not a known variable star
01:41:24.25 +43:03:13.1 -- not a known variable star
01:41:24.74 +44:25:45.4 -- not a known variable star
01:41:28.15 +50:45:37.4 -- not a known variable star
01:41:29.77 +42:45:16.0 -- not a known variable star
01:41:30.75 +43:52:17.3 -- not a known variable star
01:41:31.22 +50:15:16.3 -- not a known variable star
01:41:31.88 +43:16:12.5 -- not a known variable star
01:41:32.23 +45:53:25.1 -- not a known variable star
01:41:32.61 +49:02:41.5 -- not a known variable star
01:41:33.08 +47:09:26.5 -- not a known variable star
01:41:34.03 +47:35:43.1 -- not a known variable star
01:41:34.51 +50:12:58.6 -- not a known variable star
01:41:34.81 +50:04:10.2 -- not a known variable star
01:41:35.59 +43:18:35.1 -- not a known variable star
01:41:37.25 +49:31:01.5 -- not a known variable star
01:41:37.79 +45:33:04.7 -- not a known variable star
01:41:39.06 +48:45:55.3 -- not a known variable star
01:41:39.17 +46:45:57.0 -- not a known variable star
01:41:39.83 +43:15:07.9 -- not a known variable star
01:41:40.64 +50:38:38.2 -- not a known variable star
01:41:40.69 +49:13:48.9 -- not a known variable star
01:41:41.33 +49:43:08.2 -- not a known variable star
01:41:44.33 +48:56:42.4 -- not a known variable star
01:41:46.28 +47:10:28.5 -- not a known variable star
01:41:46.39 +44:21:09.3 -- not a known variable star
01:41:47.04 +42:49:16.7 -- not a known variable star
01:41:47.35 +42:23:36.6 -- not a known variable star
01:41:47.73 +50:48:42.9 -- not a known variable star
01:41:48.43 +46:32:32.1 -- a known variable star
01:41:50.30 +48:40:04.3 -- not a known variable star
01:41:50.50 +46:01:37.8 -- a known variable star
01:41:50.52 +48:08:44.5 -- not a known variable star
01:41:51.60 +46:18:24.2 -- not a known variable star
01:41:51.87 +44:47:41.4 -- not a known variable star
01:41:52.74 +48:30:11.1 -- not a known variable star
01:41:52.76 +43:11:19.5 -- a known variable star
01:41:52.77 +44:11:18.7 -- not a known variable star
01:41:53.55 +49:30:18.0 -- not a known variable star
01:41:56.25 +42:44:53.5 -- not a known variable star
01:41:56.40 +42:51:51.8 -- not a known variable star
01:41:58.33 +45:40:22.7 -- not a known variable star
01:41:59.00 +49:23:43.8 -- not a known variable star
01:42:00.01 +42:10:17.7 -- not a known variable star
01:42:02.82 +48:01:53.7 -- not a known variable star
01:42:02.91 +41:38:42.5 -- not a known variable star
01:42:04.22 +48:01:55.3 -- not a known variable star
01:42:06.04 +49:51:07.1 -- not a known variable star
01:42:07.84 +50:03:45.1 -- not a known variable star
01:42:08.85 +48:05:07.3 -- not a known variable star
01:42:10.20 +49:43:57.1 -- not a known variable star
01:42:11.64 +48:17:05.0 -- a known variable star
01:42:11.68 +49:58:09.9 -- not a known variable star
01:42:11.71 +43:36:15.4 -- not a known variable star
01:42:12.31 +48:06:19.6 -- not a known variable star
01:42:15.65 +41:22:02.4 -- not a known variable star
01:42:15.76 +41:27:52.2 -- not a known variable star
01:42:16.45 +46:55:29.1 -- not a known variable star
01:42:16.72 +42:18:43.8 -- a known variable star
01:42:18.20 +47:55:50.5 -- not a known variable star
01:42:19.97 +46:30:39.4 -- not a known variable star
01:42:20.08 +50:49:16.0 -- not a known variable star
01:42:22.98 +49:10:51.3 -- not a known variable star
01:42:24.03 +47:31:31.3 -- not a known variable star
01:42:24.83 +43:21:44.5 -- not a known variable star
01:42:25.29 +41:30:33.2 -- not a known variable star
01:42:25.71 +43:04:53.1 -- not a known variable star
01:42:29.49 +47:16:49.1 -- not a known variable star
01:42:31.26 +49:41:32.6 -- a known variable star
01:42:34.81 +46:57:03.4 -- not a known variable star
01:42:35.62 +43:19:12.3 -- not a known variable star
01:42:35.85 +41:06:58.6 -- not a known variable star
01:42:36.23 +48:56:29.8 -- not a known variable star
01:42:37.78 +48:32:05.4 -- not a known variable star
01:42:40.02 +48:22:31.7 -- not a known variable star
01:42:40.09 +41:50:36.9 -- not a known variable star
01:42:40.68 +42:38:43.6 -- not a known variable star
01:42:41.43 +50:53:46.8 -- not a known variable star
01:42:41.60 +41:01:11.6 -- not a known variable star
01:42:42.91 +46:13:32.6 -- not a known variable star
01:42:44.88 +50:12:26.3 -- a known variable star
01:42:45.77 +42:01:56.6 -- not a known variable star
01:42:46.68 +41:03:48.1 -- not a known variable star
01:42:46.71 +48:02:54.1 -- not a known variable star
01:42:50.32 +45:52:17.2 -- not a known variable star
01:42:50.80 +41:16:19.4 -- not a known variable star
01:42:50.83 +43:56:33.5 -- not a known variable star
01:42:51.08 +43:06:44.4 -- not a known variable star
01:42:51.28 +47:36:14.0 -- not a known variable star
01:42:51.48 +50:52:29.6 -- not a known variable star
01:42:51.60 +41:39:26.6 -- not a known variable star
01:42:53.36 +41:42:06.2 -- not a known variable star
01:42:53.39 +43:50:02.8 -- not a known variable star
01:42:53.94 +42:39:53.6 -- not a known variable star
01:42:55.31 +50:35:01.2 -- not a known variable star
01:42:55.33 +49:06:37.4 -- not a known variable star
01:42:55.50 +41:25:28.6 -- not a known variable star
01:42:57.72 +42:19:18.6 -- not a known variable star
01:43:00.68 +50:24:37.4 -- a known variable star
01:43:01.94 +43:18:08.2 -- not a known variable star
01:43:02.95 +50:49:28.9 -- not a known variable star
01:43:03.01 +45:47:14.3 -- not a known variable star
01:43:03.08 +49:14:44.3 -- not a known variable star
01:43:03.73 +50:33:40.0 -- not a known variable star
01:43:05.79 +49:47:23.6 -- not a known variable star
01:43:08.01 +41:05:22.5 -- not a known variable star
01:43:10.13 +49:54:13.0 -- not a known variable star
01:43:10.86 +49:20:43.3 -- not a known variable star
01:43:11.97 +44:52:32.4 -- not a known variable star
01:43:12.02 +50:32:39.7 -- not a known variable star
01:43:13.44 +50:03:35.0 -- not a known variable star
01:43:14.67 +42:13:52.2 -- not a known variable star
01:43:16.49 +45:50:28.8 -- not a known variable star
01:43:17.24 +44:50:12.7 -- not a known variable star
01:43:17.75 +50:48:53.9 -- not a known variable star
01:43:18.98 +50:21:32.1 -- not a known variable star
01:43:19.16 +41:23:19.1 -- not a known variable star
01:43:19.22 +44:53:54.6 -- not a known variable star
01:43:23.89 +42:07:14.2 -- not a known variable star
01:43:27.48 +50:28:06.0 -- a known variable star
01:43:28.37 +42:52:41.6 -- not a known variable star
01:43:29.86 +49:41:03.1 -- not a known variable star
01:43:31.36 +49:36:07.3 -- not a known variable star
01:43:32.43 +50:24:35.3 -- not a known variable star
01:43:35.00 +50:17:09.0 -- not a known variable star
01:43:36.69 +41:13:27.0 -- not a known variable star
01:43:37.26 +44:07:56.8 -- not a known variable star
01:43:37.77 +47:25:45.4 -- not a known variable star
01:43:37.79 +43:49:53.3 -- not a known variable star
01:43:41.87 +40:50:33.1 -- not a known variable star
01:43:42.36 +48:22:35.3 -- not a known variable star
01:43:42.62 +43:18:01.9 -- not a known variable star
01:43:43.30 +41:17:08.3 -- not a known variable star
01:43:45.28 +43:49:24.3 -- not a known variable star
01:43:48.98 +42:02:42.4 -- not a known variable star
01:43:50.29 +48:14:20.1 -- not a known variable star
01:43:52.46 +48:56:35.1 -- not a known variable star
01:43:53.92 +42:44:53.9 -- not a known variable star
01:43:55.65 +43:11:05.6 -- not a known variable star
01:43:57.46 +44:22:08.2 -- not a known variable star
01:43:58.52 +47:40:24.8 -- not a known variable star
01:44:04.60 +41:59:53.0 -- not a known variable star
01:44:04.71 +50:31:10.7 -- not a known variable star
01:44:07.77 +43:59:54.7 -- not a known variable star
01:44:08.29 +50:46:10.9 -- a known variable star
01:44:08.34 +44:31:52.3 -- not a known variable star
01:44:09.59 +48:57:04.9 -- not a known variable star
01:44:10.00 +41:26:56.9 -- not a known variable star
01:44:10.11 +45:00:10.4 -- not a known variable star
01:44:12.08 +42:09:50.1 -- not a known variable star
01:44:12.27 +50:35:01.8 -- not a known variable star
01:44:12.76 +41:15:28.4 -- not a known variable star
01:44:13.52 +50:47:28.3 -- not a known variable star
01:44:13.91 +49:20:00.7 -- not a known variable star
01:44:14.23 +47:19:45.0 -- not a known variable star
01:44:14.83 +49:40:51.5 -- not a known variable star
01:44:15.38 +42:56:25.3 -- not a known variable star
01:44:15.75 +46:40:34.7 -- not a known variable star
01:44:20.56 +44:14:23.3 -- not a known variable star
01:44:21.07 +50:27:44.5 -- a known variable star
01:44:21.12 +42:00:18.3 -- not a known variable star
01:44:22.23 +45:26:14.8 -- not a known variable star
01:44:22.30 +46:13:23.0 -- not a known variable star
01:44:23.22 +50:23:38.7 -- not a known variable star
01:44:23.44 +47:33:26.0 -- not a known variable star
01:44:24.54 +43:41:13.4 -- not a known variable star
01:44:25.79 +43:43:51.0 -- not a known variable star
01:44:27.15 +41:10:32.2 -- not a known variable star
01:44:27.99 +50:36:09.1 -- not a known variable star
01:44:28.02 +45:05:11.2 -- not a known variable star
01:44:30.20 +50:39:18.1 -- not a known variable star
01:44:31.98 +50:40:49.8 -- not a known variable star
01:44:32.18 +50:29:57.3 -- not a known variable star
01:44:33.13 +41:50:18.8 -- a known variable star
01:44:34.37 +40:54:48.1 -- not a known variable star
01:44:34.81 +42:55:59.7 -- not a known variable star
01:44:35.93 +47:22:04.6 -- not a known variable star
01:44:36.44 +41:10:50.4 -- not a known variable star
01:44:36.47 +41:24:56.4 -- not a known variable star
01:44:36.89 +50:20:54.7 -- not a known variable star
01:44:37.14 +41:48:38.2 -- not a known variable star
01:44:38.66 +40:54:01.1 -- not a known variable star
01:44:40.03 +41:26:50.8 -- not a known variable star
01:44:45.60 +43:15:53.0 -- not a known variable star
01:44:46.17 +41:07:25.0 -- not a known variable star
01:44:46.48 +50:03:43.0 -- not a known variable star
01:44:46.84 +49:40:24.1 -- not a known variable star
01:44:47.42 +50:21:23.8 -- not a known variable star
01:44:47.49 +41:00:59.5 -- not a known variable star
01:44:47.62 +47:52:24.7 -- a known variable star
01:44:48.28 +40:57:58.0 -- not a known variable star
01:44:48.52 +43:53:13.2 -- not a known variable star
01:44:48.85 +41:56:55.0 -- not a known variable star
01:44:49.63 +49:57:37.9 -- a known variable star
01:44:52.03 +41:57:29.3 -- not a known variable star
01:44:56.77 +48:16:07.7 -- a known variable star
01:44:56.88 +50:10:28.1 -- not a known variable star
01:44:58.59 +44:13:14.9 -- not a known variable star
01:45:00.36 +50:35:25.7 -- not a known variable star
01:45:06.35 +45:11:59.2 -- not a known variable star
01:45:07.56 +40:53:48.6 -- not a known variable star
01:45:11.31 +49:00:15.4 -- not a known variable star
01:45:11.61 +49:46:13.1 -- not a known variable star
01:45:13.52 +50:03:38.4 -- not a known variable star
01:45:14.26 +50:43:02.9 -- not a known variable star
01:45:14.37 +40:53:42.7 -- not a known variable star
01:45:14.42 +49:04:08.3 -- not a known variable star
01:45:15.59 +49:25:52.2 -- not a known variable star
01:45:17.34 +49:27:14.3 -- not a known variable star
01:45:17.70 +41:05:12.1 -- not a known variable star
01:45:18.13 +42:02:14.0 -- not a known variable star
01:45:19.00 +42:29:43.3 -- not a known variable star
01:45:19.09 +42:16:51.5 -- not a known variable star
01:45:19.84 +41:07:56.5 -- not a known variable star
01:45:22.30 +49:57:25.0 -- not a known variable star
01:45:23.80 +41:52:27.9 -- not a known variable star
01:45:27.42 +50:12:18.1 -- not a known variable star
01:45:29.89 +43:20:45.9 -- not a known variable star
01:45:30.58 +49:51:02.0 -- not a known variable star
01:45:30.78 +41:03:37.4 -- not a known variable star
01:45:33.11 +50:14:55.2 -- not a known variable star
01:45:34.46 +49:47:07.4 -- not a known variable star
01:45:39.66 +50:02:45.0 -- not a known variable star
01:45:44.25 +48:18:31.2 -- not a known variable star
01:45:47.48 +40:55:31.0 -- a known variable star
01:45:47.56 +44:49:48.8 -- not a known variable star
01:45:47.96 +50:04:49.7 -- not a known variable star
01:45:48.81 +44:58:04.7 -- not a known variable star
01:45:52.22 +48:57:57.0 -- not a known variable star
01:45:53.14 +49:31:40.4 -- not a known variable star
01:45:53.39 +42:19:49.6 -- not a known variable star
01:45:55.88 +50:44:39.8 -- not a known variable star
01:45:57.46 +49:08:31.1 -- not a known variable star
01:45:58.19 +41:00:40.6 -- not a known variable star
01:45:59.06 +40:53:19.0 -- not a known variable star
01:46:00.02 +42:35:07.2 -- not a known variable star
01:46:00.65 +50:03:46.1 -- not a known variable star
01:46:04.17 +42:10:40.0 -- not a known variable star
01:46:04.56 +40:54:34.9 -- a known variable star
01:46:07.54 +48:37:06.8 -- not a known variable star
01:46:08.35 +42:12:53.9 -- not a known variable star
01:46:10.89 +50:35:07.3 -- not a known variable star
01:46:10.95 +49:00:54.1 -- not a known variable star
01:46:14.29 +42:48:52.8 -- not a known variable star
01:46:16.24 +41:33:49.5 -- not a known variable star
01:46:17.19 +45:40:57.6 -- not a known variable star
01:46:23.83 +50:05:58.0 -- not a known variable star
01:46:24.88 +50:22:00.8 -- not a known variable star
01:46:25.78 +41:40:10.5 -- not a known variable star
01:46:26.56 +41:33:31.6 -- not a known variable star
01:46:27.43 +50:15:31.0 -- not a known variable star
01:46:28.14 +49:35:08.9 -- not a known variable star
01:46:28.51 +49:52:23.4 -- not a known variable star
01:46:33.45 +43:54:35.7 -- not a known variable star
01:46:37.43 +49:51:27.9 -- not a known variable star
01:46:38.45 +50:55:54.7 -- not a known variable star
01:46:38.46 +41:34:18.3 -- a known variable star
01:46:38.82 +41:54:52.4 -- not a known variable star
01:46:40.73 +49:57:41.8 -- not a known variable star
01:46:42.32 +50:10:12.3 -- not a known variable star
01:46:43.80 +41:23:12.3 -- not a known variable star
01:46:43.96 +41:33:49.0 -- not a known variable star
01:46:51.96 +48:49:14.8 -- not a known variable star
01:46:54.10 +41:10:23.1 -- not a known variable star
01:46:54.82 +50:17:09.6 -- not a known variable star
01:46:55.09 +41:29:32.4 -- not a known variable star
01:46:55.49 +43:52:12.9 -- not a known variable star
01:46:56.64 +43:04:52.0 -- not a known variable star
01:47:04.56 +47:43:42.6 -- not a known variable star
01:47:07.49 +41:16:33.6 -- not a known variable star
01:47:07.75 +49:19:04.6 -- not a known variable star
01:47:08.56 +49:42:19.1 -- not a known variable star
01:47:08.59 +48:09:21.2 -- not a known variable star
01:47:08.66 +40:59:47.9 -- not a known variable star
01:47:12.50 +42:46:55.2 -- not a known variable star
01:47:13.39 +50:08:57.4 -- not a known variable star
01:47:18.94 +49:50:41.9 -- not a known variable star
01:47:21.67 +40:56:47.3 -- not a known variable star
01:47:23.38 +40:55:35.7 -- not a known variable star
01:47:23.85 +49:04:34.6 -- not a known variable star
01:47:26.71 +49:57:44.8 -- not a known variable star
01:47:27.45 +49:45:10.3 -- not a known variable star
01:47:28.81 +41:22:25.3 -- a known variable star
01:47:29.12 +49:53:59.1 -- not a known variable star
01:47:29.28 +41:23:13.3 -- not a known variable star
01:47:31.65 +41:51:38.2 -- not a known variable star
01:47:32.15 +41:04:11.7 -- a known variable star
01:47:37.68 +41:35:32.3 -- not a known variable star
01:47:39.04 +41:09:46.3 -- not a known variable star
01:47:43.06 +41:11:40.9 -- not a known variable star
01:47:43.77 +41:03:06.3 -- not a known variable star
01:48:01.18 +40:58:04.6 -- not a known variable star
01:48:01.76 +49:58:50.0 -- not a known variable star
01:48:07.32 +50:18:38.5 -- not a known variable star
01:48:08.64 +49:34:01.7 -- not a known variable star
01:48:09.36 +50:53:40.7 -- not a known variable star
01:48:14.51 +41:15:36.5 -- not a known variable star
01:48:15.53 +41:20:03.0 -- not a known variable star
01:48:16.75 +42:23:33.7 -- not a known variable star
01:48:18.99 +49:06:03.5 -- not a known variable star
01:48:20.88 +50:22:19.2 -- not a known variable star
01:48:29.42 +41:01:54.5 -- not a known variable star
01:48:38.44 +50:20:15.2 -- not a known variable star
01:48:45.20 +50:33:06.6 -- not a known variable star
01:48:59.66 +48:12:09.0 -- a known variable star
01:49:01.06 +41:15:55.0 -- not a known variable star
01:49:03.79 +41:05:49.8 -- not a known variable star
01:49:10.98 +50:08:40.1 -- not a known variable star
01:49:28.57 +41:36:46.3 -- not a known variable star
01:49:44.56 +49:53:47.1 -- a known variable star
01:49:50.70 +49:46:20.0 -- not a known variable star
01:49:57.88 +49:25:13.3 -- not a known variable star
01:49:58.89 +50:47:44.2 -- not a known variable star
01:50:37.60 +50:34:55.7 -- not a known variable star
01:50:45.68 +49:47:12.6 -- not a known variable star
01:51:10.81 +50:11:41.3 -- not a known variable star
01:51:11.71 +41:34:55.6 -- not a known variable star
01:51:13.32 +50:27:20.2 -- not a known variable star
01:51:13.71 +50:00:48.0 -- not a known variable star
01:51:14.68 +50:50:07.4 -- not a known variable star
01:51:15.90 +49:44:40.3 -- not a known variable star
01:51:28.58 +50:40:50.0 -- not a known variable star
01:52:01.75 +50:43:20.4 -- not a known variable star
01:52:40.28 +41:27:03.3 -- not a known variable star
01:53:01.77 +50:59:18.7 -- not a known variable star
01:53:18.35 +50:20:13.6 -- not a known variable star
01:54:13.09 +50:55:58.7 -- not a known variable star
01:56:48.56 +43:10:17.5 -- not a known variable star
01:59:16.34 +50:55:48.0 -- not a known variable star
02:11:02.76 +48:56:44.2 -- a known variable star
02:13:12.76 +49:57:24.7 -- not a known variable star
02:15:26.80 +47:49:30.1 -- not a known variable star
02:18:18.35 +49:53:11.9 -- not a known variable star
02:18:55.22 +45:28:22.0 -- a known variable star
02:22:26.91 +42:18:07.3 -- not a known variable star
02:23:03.21 +48:12:01.7 -- a known variable star
02:25:53.93 +46:25:30.0 -- not a known variable star
02:28:25.37 +45:36:03.5 -- not a known variable star
02:32:11.23 +49:54:37.5 -- a known variable star
02:32:46.05 +46:29:20.8 -- a known variable star
02:32:53.71 +48:20:16.8 -- a known variable star
02:33:46.26 +48:29:08.9 -- a known variable star
02:33:48.96 +45:12:54.0 -- a known variable star
02:35:51.44 +49:18:00.8 -- a known variable star
02:36:24.20 +44:54:58.7 -- not a known variable star
02:38:12.61 +47:05:58.4 -- not a known variable star
02:48:15.68 +44:37:04.6 -- a known variable star
02:52:22.70 +48:39:52.3 -- a known variable star
02:56:41.72 +50:33:24.5 -- a known variable star
02:59:56.11 +42:37:15.3 -- a known variable star
Found 409 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
452 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
No ../exclusion_list_TTUQ2.txt so we are not updating exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= YES
The observatory MPC code is 500
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.68004000 -observatory 500
23:23:27.55 -01:58:30.4 Mercury (-0.1mag)
23:04:31.26 -07:29:28.1 Venus (-3.9mag)
21:42:50.98 -14:52:39.2 Mars (1.1mag)
07:06:05.85 +22:54:20.3 Jupiter (-2.5mag)
00:05:26.49 -01:44:26.0 Saturn (1.0mag)
03:39:59.54 +19:21:43.9 Uranus (5.7mag)
00:03:40.99 -01:01:36.8 Neptune (7.8mag)
20:29:07.14 -22:59:34.0 Pluto (14.5mag)
01:54:54.61 +16:19:25.5 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 21 22:31 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.68004000:
07:06:10.58 +22:54:13.5 Io (5.4mag)
07:06:17.69 +22:53:58.4 Europa (5.5mag)
07:05:57.06 +22:54:45.1 Ganymede (4.9mag)
07:06:25.19 +22:53:54.2 Callisto (6.2mag)
07:09:14.89 +23:10:42.8 Himalia (15.0mag)
07:06:08.11 +22:54:18.2 Thebe (15.9mag)
07:08:39.95 +23:19:12.1 Elara (17.0mag)
07:01:39.45 +24:02:18.1 Pasiphae (17.0mag)
07:15:06.73 +22:42:20.7 Carme (18.1mag)
00:05:38.21 -01:44:30.5 Titan (8.8mag)
00:05:32.01 -01:44:24.6 Rhea (10.1mag)
00:05:21.93 -01:45:46.8 Iapetus (11.5mag)
00:05:27.40 -01:44:29.1 Hyperion (14.8mag)
00:07:30.76 -01:31:26.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 21 22:31 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.68004000:
08:45:58.86 +24:30:44.4 JWST
12:10:51.26 +51:13:32.5 Chandra
15:42:14.20 -58:04:53.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 21 22:31 spacecraft.txt
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Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461093.68004000 at 500
16:59:44.59 -11:03:50.4 17.5mag 10P/Tempel 2
03:37:20.22 +28:57:54.7 18.0mag 123P/West-Hartley
08:23:36.35 +60:42:26.3 18.4mag 124P/Mrkos
21:19:39.69 -07:38:21.5 22.1mag 141P/Machholz
01:21:12.35 +11:55:16.9 17.7mag 145P/Shoemaker-Levy 5
11:02:57.57 +30:34:42.6 17.9mag 164P/Christensen
04:45:18.54 +19:21:01.8 0.0mag 195P/Hill
15:52:03.07 -06:35:44.3 19.2mag 210P/Christensen
18:16:58.57 -21:28:25.4 17.3mag 218P/LINEAR
16:21:36.75 -18:10:54.1 15.2mag 235P/LINEAR
03:56:25.55 +27:44:47.6 17.8mag 240P/NEAT
15:17:39.62 +06:38:18.2 14.8mag 24P/Schaumasse
11:23:30.46 -03:23:07.2 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.67 +27:24:50.5 19.6mag 407P/PanSTARRS-Fuls
17:07:11.30 -11:19:13.5 17.6mag 40P/Vaisala 1
11:02:11.86 -08:51:47.7 16.6mag 43P/Wolf-Harrington
04:45:18.54 +19:21:01.8 0.0mag 489P/Denning
04:34:23.26 +48:34:26.4 17.8mag 493P/2024 Q2 (LONEOS)
06:04:23.79 +47:31:10.4 17.7mag 63P/Wild 1
23:14:39.60 -02:07:13.8 16.2mag 78P/Gehrels 2
20:01:36.11 -22:18:04.5 15.0mag 88P/Howell
15:27:55.45 -29:00:48.3 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.26 -72:35:48.9 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:49.76 +31:12:54.4 18.2mag C/2017 K2 (PanSTARRS)
20:06:39.13 -65:11:41.1 18.1mag C/2020 V2 (ZTF)
17:21:41.08 +04:21:33.0 16.3mag C/2021 G2 (ATLAS)
03:35:42.28 +24:36:44.2 15.8mag C/2022 N2 (PanSTARRS)
09:08:12.70 +29:49:42.3 15.3mag C/2022 QE78 (ATLAS)
08:35:40.07 -06:33:35.1 16.7mag C/2022 R6 (PanSTARRS)
23:53:04.18 +48:26:49.4 18.0mag C/2023 C2 (ATLAS)
09:51:06.05 -20:45:45.1 17.5mag C/2023 F3 (ATLAS)
20:34:48.52 +61:14:31.0 17.3mag C/2023 H5 (Lemmon)
19:34:30.32 -03:24:16.7 16.1mag C/2023 R1 (PANSTARRS)
02:48:55.83 +35:40:33.5 18.5mag C/2023 RS61 (PanSTARRS)
21:01:29.79 +81:19:58.6 18.0mag C/2023 X2 (Lemmon)
06:39:07.38 +63:49:15.7 17.3mag C/2024 A1 (ATLAS)
01:56:57.30 -24:35:34.7 11.2mag C/2024 E1 (Wierzchos)
11:44:57.40 -02:34:32.4 18.1mag C/2024 G2 (ATLAS)
19:28:20.56 +00:39:15.9 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.68 -01:42:40.0 17.7mag C/2024 G6 (ATLAS)
19:53:28.72 +03:15:25.0 15.6mag C/2024 J3 (ATLAS)
02:47:15.48 -31:34:10.1 15.4mag C/2024 T5 (ATLAS)
16:25:01.55 -58:14:27.2 15.6mag C/2025 A6 (Lemmon)
04:50:29.17 +62:13:51.4 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
15:56:42.29 -12:59:54.0 14.8mag C/2025 L1 (ATLAS)
02:20:15.49 -19:06:12.1 16.7mag C/2025 Q3 (ATLAS)
02:09:36.63 +17:16:53.5 21.2mag C/2025 R2 (SWAN)
22:20:46.46 +17:39:17.1 16.4mag C/2025 R3 (PANSTARRS)
21:46:03.01 -16:50:46.4 21.5mag C/2025 T1 (ATLAS)
03:06:10.62 -20:33:13.4 18.3mag C/2026 A1 (MAPS)
21:03:08.20 +20:56:23.0 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 21 22:32 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
-rw-r--r-- 1 apache apache 6.2K Feb 21 22:31 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 21 22:31 tocp_transients_list.txt