This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 29 32.62 +49 25 24.8 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391603027721688704,2461093.6516,11.13,0.05,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 391603027721688704 20260222.1516 11.13CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:32.62 +49:25:24.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.19 00:44:52.14 +46:14:18.9
121.74663 -16.61805 galactic And Second-epoch detections are separated by 2.3" 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 J011.2241+46.2531 | 00:44:53.44 +46:14:42.2 (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 22.1516* 00 44 52.14 +46 14 18.9 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
ATO J011.2241+46.2531,2461093.6516,11.19,0.05,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
ATO J011.2241+46.2531 20260222.1516 11.19CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:52.14 +46:14:18.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.11 00:34:34.69 +42:09:25.3
119.59492 -20.60545 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 | ATO J008.6489+42.1647 | 00:34:33.79 +42:09:18.2 (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 22.1516* 00 34 34.69 +42 09 25.3 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
ATO J008.6489+42.1647,2461093.6516,11.11,0.05,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
ATO J008.6489+42.1647 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:34.69 +42:09:25.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.00 00:54:37.50 +49:28:21.1
123.46414 -13.39593 galactic Cas Second-epoch detections are separated by 7.7" 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 | ATO J013.6387+49.4769 | 00:54:35.50 +49:28:20.5 (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 22.1516* 00 54 37.50 +49 28 21.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J013.6387+49.4769,2461093.6516,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J013.6387+49.4769 20260222.1516 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:54:37.50 +49:28:21.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.04 00:38:39.17 +43:48:36.1
120.49297 -19.00117 galactic And Second-epoch detections are separated by 3.2" 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 varaible 387754565222316416 | 00:38:39.53 +43:48:41.4 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 38 39.17 +43 48 36.1 11.0 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 varaible 387754565222316416,2461093.6516,11.04,0.05,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
Gaia DR3 varaible 387754565222316416 20260222.1516 11.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:39.17 +43:48:36.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.88 00:33:45.23 +42:24:49.0
119.45219 -20.33862 galactic And Second-epoch detections are separated by 1.4" 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 varaible 382281677375410944 | 00:33:44.27 +42:24:44.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 33 45.23 +42 24 49.0 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 varaible 382281677375410944,2461093.6516,10.88,0.05,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 varaible 382281677375410944 20260222.1516 10.88CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:45.23 +42:24:49.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.55 00:35:55.68 +42:23:43.1
119.87794 -20.38445 galactic And Second-epoch detections are separated by 4.1" 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 | Gaia DR3 varaible 381615338967873664 | 00:35:54.95 +42:23:39.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 35 55.68 +42 23 43.1 10.6 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 varaible 381615338967873664,2461093.6516,10.55,0.05,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 varaible 381615338967873664 20260222.1516 10.55CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:55.68 +42:23:43.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.67 00:40:58.52 +41:43:55.5
120.83997 -21.09716 galactic And Second-epoch detections are separated by 1.1" 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 varaible 381335783844895744 | 00:40:57.98 +41:43:50.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 40 58.52 +41 43 55.5 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 varaible 381335783844895744,2461093.6516,10.67,0.05,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 varaible 381335783844895744 20260222.1516 10.67CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:58.52 +41:43:55.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.52 00:42:32.09 +40:57:18.8
121.12057 -21.88521 galactic And Second-epoch detections are separated by 3.7" 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 J010.6389+40.9556 | 00:42:31.21 +40:57:12.6 (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 22.1516* 00 42 32.09 +40 57 18.8 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
ATO J010.6389+40.9556,2461093.6516,10.52,0.05,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
ATO J010.6389+40.9556 20260222.1516 10.52CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:32.09 +40:57:18.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.54 00:39:19.95 +41:55:34.6
120.52230 -20.88883 galactic And Second-epoch detections are separated by 3.4" 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 | Gaia DR3 varaible 381540125502188416 | 00:39:19.52 +41:55:31.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 39 19.95 +41 55 34.6 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 varaible 381540125502188416,2461093.6516,10.54,0.05,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 varaible 381540125502188416 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:19.95 +41:55:34.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.43 00:46:22.18 +50:04:38.5
122.09814 -12.78618 galactic Cas Second-epoch detections are separated by 1.9" 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 414765747689792128 | 00:46:23.26 +50:04:34.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1952CoRut..32....1H BD+49 183
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 46 22.18 +50 04 38.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414765747689792128,2461093.6516,10.43,0.05,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 414765747689792128 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:22.18 +50:04:38.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.39 00:52:57.44 +50:46:08.6
123.17761 -12.10197 galactic Cas Second-epoch detections are separated by 4.5" and 4.8 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 J013.2247+50.7722 | 00:52:57.90 +50:46:02.7 (Gaia DR3) | CBH (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F8 1927AnHar.100...33C HD 232298
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 52 57.44 +50 46 08.6 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J013.2247+50.7722,2461093.6516,10.39,0.05,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 J013.2247+50.7722 20260222.1516 10.39CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:52:57.44 +50:46:08.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 33 22.70 +49 51 24.6 10.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391675183171249408,2461093.6516,10.29,0.05,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
Gaia DR3 391675183171249408 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:22.70 +49:51:24.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.54 00:34:27.80 +49:19:12.3
120.08910 -13.45795 galactic Cas Second-epoch detections are separated by 2.9" 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 | Gaia DR3 391376322166687744 | 00:34:29.22 +49:19:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1952CoRut..32....1H BD+48 169
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 34 27.80 +49 19 12.3 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391376322166687744,2461093.6516,10.54,0.05,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 391376322166687744 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:27.80 +49:19:12.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.44 00:40:15.19 +50:49:23.2
121.12641 -12.00942 galactic Cas Second-epoch detections are separated by 7.2" and 3.9 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 415608596370233856 | 00:40:16.06 +50:49:22.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1927AnHar.100...33C HD 232244
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 40 15.19 +50 49 23.2 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415608596370233856,2461093.6516,10.44,0.05,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 415608596370233856 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:15.19 +50:49:23.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.56 00:42:38.80 +49:34:51.5
121.46805 -13.26579 galactic Cas Second-epoch detections are separated by 5.9" and 4.5 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 J010.6532+49.5767 | 00:42:39.89 +49:34:51.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 1952CoRut..32....1H BD+48 212
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 42 38.80 +49 34 51.5 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J010.6532+49.5767,2461093.6516,10.56,0.05,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 J010.6532+49.5767 20260222.1516 10.56CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:38.80 +49:34:51.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.59 00:28:11.05 +50:28:08.9
119.14950 -12.23175 galactic Cas Second-epoch detections are separated by 1.1" 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 391763964436082816 | 00:28:11.70 +50:28:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1952CoRut..32....1H BD+49 97
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 28 11.05 +50 28 08.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391763964436082816,2461093.6516,10.59,0.05,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 391763964436082816 20260222.1516 10.59CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:11.05 +50:28:08.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.62 00:33:55.33 +48:39:10.4
119.95057 -14.11744 galactic Cas Second-epoch detections are separated by 5.0" 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 390960947289675904 | 00:33:56.23 +48:39:14.5 (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 22.1516* 00 33 55.33 +48 39 10.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390960947289675904,2461093.6516,10.62,0.05,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 390960947289675904 20260222.1516 10.62CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:55.33 +48:39:10.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.85 00:35:43.70 +41:45:08.4
119.79390 -21.02368 galactic And Second-epoch detections are separated by 3.4" 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 varaible 381479755441227648 | 00:35:44.11 +41:45:24.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 35 43.70 +41 45 08.4 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
Gaia DR3 varaible 381479755441227648,2461093.6516,10.85,0.05,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
Gaia DR3 varaible 381479755441227648 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:43.70 +41:45:08.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.79 00:28:05.04 +49:10:14.5
119.00955 -13.52311 galactic Cas Second-epoch detections are separated by 4.0" 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 391221394106034048 | 00:28:06.00 +49:10:11.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1952CoRut..32....1H BD+48 135
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 28 05.04 +49 10 14.5 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391221394106034048,2461093.6516,10.79,0.05,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 391221394106034048 20260222.1516 10.79CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:05.04 +49:10:14.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 31 28.44 +49 04 22.2 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391161951761028480,2461093.6516,10.81,0.05,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 391161951761028480 20260222.1516 10.81CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:28.44 +49:04:22.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.84 00:36:27.59 +50:58:06.8
120.52362 -11.83314 galactic Cas Second-epoch detections are separated by 2.4" and 5.3 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 415579287512630784 | 00:36:28.40 +50:58:01.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1956PMcCO..13a....B AG+50 54
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 36 27.59 +50 58 06.8 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415579287512630784,2461093.6516,10.84,0.05,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 415579287512630784 20260222.1516 10.84CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:27.59 +50:58:06.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.84 00:25:16.24 +50:31:57.6
118.68419 -12.12314 galactic Cas Second-epoch detections are separated by 5.7" and 5.3 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 J006.3319+50.5379 | 00:25:17.38 +50:31:49.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1956PMcCO..13a....B AG+50 37
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 25 16.24 +50 31 57.6 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.3319+50.5379,2461093.6516,10.84,0.05,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
ATO J006.3319+50.5379 20260222.1516 10.84CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:25:16.24 +50:31:57.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.00 00:46:51.43 +42:18:06.4
122.02732 -20.56193 galactic And Second-epoch detections are separated by 4.1" 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 varaible 375338776842857856 | 00:46:49.45 +42:17:51.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 46 51.43 +42 18 06.4 11.0 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 varaible 375338776842857856,2461093.6516,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 varaible 375338776842857856 20260222.1516 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:51.43 +42:18:06.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 32 50.53 +49 19 44.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0381 Cas,2461093.6516,11.04,0.05,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
V0381 Cas 20260222.1516 11.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:50.53 +49:19:44.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.17 00:26:49.68 +50:46:16.7
118.95983 -11.91054 galactic Cas Second-epoch detections are separated by 5.2" and 5.3 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 394778726539074688 | 00:26:50.40 +50:46:12.5 (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 22.1516* 00 26 49.68 +50 46 16.7 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394778726539074688,2461093.6516,11.17,0.05,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 394778726539074688 20260222.1516 11.17CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:49.68 +50:46:16.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.17 00:55:15.09 +49:39:22.0
123.56588 -13.21094 galactic Cas Second-epoch detections are separated by 5.8" 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 402869482851365248 | 00:55:15.99 +49:39:07.4 (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 22.1516* 00 55 15.09 +49 39 22.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 402869482851365248,2461093.6516,11.17,0.05,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 402869482851365248 20260222.1516 11.17CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:55:15.09 +49:39:22.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.30 00:36:48.66 +50:42:52.3
120.56495 -12.08999 galactic Cas Second-epoch detections are separated by 2.1" 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 415566814930124160 | 00:36:49.52 +50:42:56.9 (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 22.1516* 00 36 48.66 +50 42 52.3 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415566814930124160,2461093.6516,11.30,0.05,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 415566814930124160 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:48.66 +50:42:52.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.28 00:31:44.18 +50:02:56.2
119.69212 -12.69883 galactic Cas Second-epoch detections are separated by 2.8" 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 391692427461219584 | 00:31:44.87 +50:02:56.1 (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 22.1516* 00 31 44.18 +50 02 56.2 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391692427461219584,2461093.6516,11.28,0.05,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 391692427461219584 20260222.1516 11.28CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:44.18 +50:02:56.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 31 58.34 +45 46 20.7 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
EO And,2461093.6516,11.68,0.05,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
EO And 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:31:58.34 +45:46:20.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 16 19.81 +47 27 31.0 11.0 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
ASASSN-V J011619.80+472731.5,2461093.6516,11.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J011619.80+472731.5 20260222.1516 11.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:16:19.81 +47:27:31.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 15 42.26 +46 12 18.4 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
ASASSN-V J011542.35+461218.2,2461093.6516,10.40,0.05,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
ASASSN-V J011542.35+461218.2 20260222.1516 10.40CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:15:42.26 +46:12:18.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 25 48.53 +46 24 13.0 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
NSVS J0125488+462415,2461093.6516,10.87,0.05,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
NSVS J0125488+462415 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:25:48.53 +46:24:13.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 14 04.52 +47 52 07.5 10.3 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
ASASSN-V J011404.54+475208.8,2461093.6516,10.31,0.05,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
ASASSN-V J011404.54+475208.8 20260222.1516 10.31CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:14:04.52 +47:52:07.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 10 12.93 +49 10 15.4 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J0110132+491018,2461093.6516,10.62,0.05,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
NSVS J0110132+491018 20260222.1516 10.62CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:10:12.93 +49:10:15.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 58 20.83 +49 25 06.4 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J005820.24+492513.7,2461093.6516,11.01,0.05,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
ASASSN-V J005820.24+492513.7 20260222.1516 11.01CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:58:20.83 +49:25:06.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 45 56.25 +50 23 15.7 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J0045548+502335,2461093.6516,11.46,0.05,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
NSVS J0045548+502335 20260222.1516 11.46CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:56.25 +50:23:15.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 26 27.60 +49 53 58.1 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
ASASSN-V J012627.86+495401.2,2461093.6516,10.44,0.05,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
ASASSN-V J012627.86+495401.2 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:26:27.60 +49:53:58.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 33 35.62 +46 31 13.7 9.1 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
SX And,2461093.6516,9.12,0.05,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
SX And 20260222.1516 9.12CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:33:35.62 +46:31:13.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.39 00:40:54.80 +43:18:07.5
120.90053 -19.52815 galactic And Second-epoch detections are separated by 6.4" 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 varaible 387449377730838016 | 00:40:55.08 +43:18:14.4 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 40 54.80 +43 18 07.5 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 varaible 387449377730838016,2461093.6516,13.39,0.05,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 varaible 387449377730838016 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:54.80 +43:18:07.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.34 00:41:27.98 +44:06:28.9
121.04214 -18.72713 galactic And Second-epoch detections are separated by 3.6" and 5.3 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 | 00:41:27.98 +44:06:28.9 (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 22.1516* 00 41 27.98 +44 06 28.9 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
target,2461093.6516,13.34,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:27.98 +44:06:28.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.66 01:00:20.71 +41:01:19.8
124.74142 -21.81828 galactic And Second-epoch detections are separated by 1.4" 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 | target | 01:00:20.71 +41:01:19.8 (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 22.1516* 01 00 20.71 +41 01 19.8 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,2461093.6516,13.66,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:00:20.71 +41:01:19.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.43 00:45:14.07 +41:03:01.6
121.67229 -21.80613 galactic And Second-epoch detections are separated by 7.8" and 4.7 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 varaible 369213530706029440 | 00:45:14.71 +41:03:08.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 45 14.07 +41 03 01.6 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 varaible 369213530706029440,2461093.6516,13.43,0.05,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 varaible 369213530706029440 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:14.07 +41:03:01.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.15 00:29:49.36 +41:44:42.3
118.61710 -20.94550 galactic And Second-epoch detections are separated by 7.2" 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 | Gaia DR3 varaible 381904643669634688 | 00:29:50.11 +41:44:50.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 29 49.36 +41 44 42.3 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 varaible 381904643669634688,2461093.6516,13.15,0.05,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 varaible 381904643669634688 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:49.36 +41:44:42.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.30 00:44:05.02 +42:19:57.0
121.48079 -20.51853 galactic And Second-epoch detections are separated by 3.9" 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 | target | 00:44:05.02 +42:19:57.0 (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 22.1516* 00 44 05.02 +42 19 57.0 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,2461093.6516,13.30,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:05.02 +42:19:57.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 29 26.69 +46 27 24.0 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 398929726529571072,2461093.6516,13.69,0.05,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 398929726529571072 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:29:26.69 +46:27:24.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.59 01:28:47.66 +44:16:39.2
129.95232 -18.08438 galactic And Second-epoch detections are separated by 5.4" 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 | target | 01:28:47.66 +44:16:39.2 (user input) | T | P | (position from user input) SpType: K5 (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 22.1516* 01 28 47.66 +44 16 39.2 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
target,2461093.6516,13.59,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:28:47.66 +44:16:39.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.36 00:56:54.71 +41:31:41.7
124.03171 -21.33181 galactic And Second-epoch detections are separated by 5.8" 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 varaible 374343650098456320 | 00:56:54.71 +41:31:41.7 (user input) | | 2022yCat.1358....0G | (position from user input) Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 56 54.71 +41 31 41.7 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 varaible 374343650098456320,2461093.6516,13.36,0.05,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 varaible 374343650098456320 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:56:54.71 +41:31:41.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 46 26.17 +45 54 34.7 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
target,2461093.6516,13.22,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:26.17 +45:54:34.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.21 00:32:49.44 +41:33:51.5
119.19955 -21.17251 galactic And Second-epoch detections are separated by 3.8" and 4.6 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 varaible 381858365398660352 | 00:32:50.08 +41:33:56.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 32 49.44 +41 33 51.5 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 varaible 381858365398660352,2461093.6516,13.21,0.05,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 varaible 381858365398660352 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:49.44 +41:33:51.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.38 00:42:36.20 +44:15:33.5
121.26327 -18.58382 galactic And Second-epoch detections are separated by 2.9" 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 | target | 00:42:36.20 +44:15:33.5 (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 22.1516* 00 42 36.20 +44 15 33.5 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
target,2461093.6516,13.38,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:36.20 +44:15:33.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.60 01:51:23.52 +49:56:14.5
132.72241 -11.79125 galactic Per Second-epoch detections are separated by 1.7" 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 | target | 01:51:23.52 +49:56:14.5 (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 22.1516* 01 51 23.52 +49 56 14.5 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
target,2461093.6516,13.60,0.05,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 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:23.52 +49:56:14.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.18 00:39:05.16 +40:55:41.8
120.41811 -21.88317 galactic And Second-epoch detections are separated by 1.5" 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 | Gaia DR3 varaible 381151585581580800 | 00:39:05.47 +40:55:48.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 39 05.16 +40 55 41.8 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 varaible 381151585581580800,2461093.6516,13.18,0.05,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 varaible 381151585581580800 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:05.16 +40:55:41.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.03 00:30:50.10 +41:16:32.5
118.77538 -21.42972 galactic And Second-epoch detections are separated by 4.4" 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 J007.7192+41.2759 | 00:30:50.58 +41:16:36.0 (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 22.1516* 00 30 50.10 +41 16 32.5 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 J007.7192+41.2759,2461093.6516,13.03,0.05,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
ATO J007.7192+41.2759 20260222.1516 13.03CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:50.10 +41:16:32.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.27 00:40:06.38 +42:22:42.1
120.69890 -20.44425 galactic And Second-epoch detections are separated by 1.5" 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 varaible 381395333574185728 | 00:40:06.84 +42:22:53.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 40 06.38 +42 22 42.1 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 varaible 381395333574185728,2461093.6516,13.27,0.05,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 varaible 381395333574185728 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:06.38 +42:22:42.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.11 00:32:34.15 +48:41:56.2
119.72436 -14.05526 galactic Cas Second-epoch detections are separated by 8.9" 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 | ATO J008.1448+48.6990 | 00:32:34.77 +48:41:56.6 (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 22.1516* 00 32 34.15 +48 41 56.2 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J008.1448+48.6990,2461093.6516,13.11,0.05,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
ATO J008.1448+48.6990 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:34.15 +48:41:56.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 42 10.50 +41 26 20.5 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
target,2461093.6516,13.29,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:10.50 +41:26:20.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.24 00:39:18.12 +49:31:27.4
120.90873 -13.29979 galactic Cas Second-epoch detections are separated by 5.6" 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 | Large-amplitude variable Gaia DR2 391430060798072576 | 00:39:18.59 +49:31:23.6 (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 22.1516* 00 39 18.12 +49 31 27.4 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 391430060798072576,2461093.6516,13.24,0.05,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
Large-amplitude variable Gaia DR2 391430060798072576 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:18.12 +49:31:27.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.12 00:46:32.24 +41:51:49.3
121.95463 -20.99875 galactic And Second-epoch detections are separated by 5.6" 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 | ATO J011.6346+41.8655 | 00:46:32.31 +41:51:56.1 (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 22.1516* 00 46 32.24 +41 51 49.3 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 J011.6346+41.8655,2461093.6516,13.12,0.05,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 J011.6346+41.8655 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:32.24 +41:51:49.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.04 00:31:15.32 +44:21:00.0
119.13219 -18.37280 galactic And Second-epoch detections are separated by 3.5" 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 | Gaia DR3 varaible 388523295649115520 | 00:31:15.79 +44:21:03.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 31 15.32 +44 21 00.0 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 varaible 388523295649115520,2461093.6516,13.04,0.05,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
Gaia DR3 varaible 388523295649115520 20260222.1516 13.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:15.32 +44:21:00.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.05 00:31:08.32 +42:49:07.5
118.97522 -19.89699 galactic And Second-epoch detections are separated by 0.9" 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 varaible 382352419780672256 | 00:31:08.87 +42:49:00.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 31 08.32 +42 49 07.5 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 varaible 382352419780672256,2461093.6516,13.05,0.05,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 varaible 382352419780672256 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:08.32 +42:49:07.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.08 00:42:58.20 +40:58:58.5
121.21011 -21.86052 galactic And Second-epoch detections are separated by 2.2" and 6.0 pix This object is listed in tocp_transients_list.txt 9.7" PNV J00425751+4059043 2022-02-16.4234 16.0mag
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 | 00:42:58.20 +40:58:58.5 (user input) | T | P | (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 22.1516* 00 42 58.20 +40 58 58.5 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
target,2461093.6516,13.08,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:58.20 +40:58:58.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.03 00:29:18.89 +46:12:00.8
118.94241 -16.50008 galactic And Second-epoch detections are separated by 6.2" 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 varaible 389294671776774400 | 00:29:19.71 +46:12:03.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 29 18.89 +46 12 00.8 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 varaible 389294671776774400,2461093.6516,13.03,0.05,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 varaible 389294671776774400 20260222.1516 13.03CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:18.89 +46:12:00.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.25 00:38:14.08 +42:16:52.0
120.32483 -20.52379 galactic And Second-epoch detections are separated by 4.0" 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 | Gaia DR3 varaible 381566337686192896 | 00:38:14.00 +42:16:58.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 38 14.08 +42 16 52.0 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 varaible 381566337686192896,2461093.6516,13.25,0.05,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 varaible 381566337686192896 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:14.08 +42:16:52.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.27 01:21:11.80 +48:29:08.2
128.00838 -14.09260 galactic And Second-epoch detections are separated by 1.7" 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 | ATO J020.2939+48.4891 | 01:21:11.80 +48:29:08.2 (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 22.1516* 01 21 11.80 +48 29 08.2 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
ATO J020.2939+48.4891,2461093.6516,13.27,0.05,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 J020.2939+48.4891 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:21:11.80 +48:29:08.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.12 00:40:19.55 +43:04:59.3
120.77658 -19.74210 galactic And Second-epoch detections are separated by 1.0" 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 | Gaia DR3 varaible 387626811419696512 | 00:40:19.95 +43:05:07.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 40 19.55 +43 04 59.3 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 varaible 387626811419696512,2461093.6516,13.12,0.05,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 varaible 387626811419696512 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:19.55 +43:04:59.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.04 00:30:51.74 +41:44:46.9
118.82408 -20.96122 galactic And Second-epoch detections are separated by 4.3" 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 varaible 381855715402221952 | 00:30:52.78 +41:44:55.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 30 51.74 +41 44 46.9 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 varaible 381855715402221952,2461093.6516,13.04,0.05,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
Gaia DR3 varaible 381855715402221952 20260222.1516 13.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:51.74 +41:44:46.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.09 00:43:44.55 +41:04:55.1
121.37054 -21.76645 galactic And Second-epoch detections are separated by 8.3" 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 J010.9348+41.0879 | 00:43:44.66 +41:05:01.9 (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 22.1516* 00 43 44.55 +41 04 55.1 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
ATO J010.9348+41.0879,2461093.6516,13.09,0.05,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
ATO J010.9348+41.0879 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:44.55 +41:04:55.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.02 00:36:25.74 +42:34:30.4
119.98832 -20.21084 galactic And Second-epoch detections are separated by 3.5" 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 varaible 381620522993578624 | 00:36:26.02 +42:34:35.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 36 25.74 +42 34 30.4 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 varaible 381620522993578624,2461093.6516,13.02,0.05,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 varaible 381620522993578624 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:25.74 +42:34:30.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.04 00:49:17.74 +42:47:31.3
122.51348 -20.07798 galactic And Second-epoch detections are separated by 6.4" 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 | target | 00:49:17.74 +42:47:31.3 (user input) | T | P | (position from user input) 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 22.1516* 00 49 17.74 +42 47 31.3 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
target,2461093.6516,13.04,0.05,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 20260222.1516 13.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:49:17.74 +42:47:31.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.06 00:40:33.46 +44:20:49.8
120.88131 -18.48126 galactic And Second-epoch detections are separated by 5.6" 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 | ATO J010.1349+44.3507 | 00:40:33.18 +44:20:55.1 (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 22.1516* 00 40 33.46 +44 20 49.8 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
ATO J010.1349+44.3507,2461093.6516,13.06,0.05,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 J010.1349+44.3507 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:33.46 +44:20:49.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.18 00:30:55.16 +50:04:24.3
119.56015 -12.66395 galactic Cas Second-epoch detections are separated by 8.1" and 5.0 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 J007.7159+50.0705 | 00:30:55.45 +50:04:12.1 (Gaia DR3) | CBF (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 22.1516* 00 30 55.16 +50 04 24.3 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J007.7159+50.0705,2461093.6516,13.18,0.05,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
ATO J007.7159+50.0705 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:55.16 +50:04:24.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.93 00:40:14.45 +44:46:47.0
120.84250 -18.04660 galactic And Second-epoch detections are separated by 0.4" 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 varaible 388183267381905792 | 00:40:15.27 +44:46:48.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 40 14.45 +44 46 47.0 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 varaible 388183267381905792,2461093.6516,12.93,0.05,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 varaible 388183267381905792 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:14.45 +44:46:47.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.21 00:42:21.35 +45:04:14.7
121.24825 -17.77131 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 | Gaia DR3 varaible 388108951563720960 | 00:42:21.96 +45:04:25.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 42 21.35 +45 04 14.7 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 varaible 388108951563720960,2461093.6516,13.21,0.05,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 varaible 388108951563720960 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:21.35 +45:04:14.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.02 00:39:07.27 +48:10:19.6
120.80996 -14.64888 galactic Cas Second-epoch detections are separated by 3.5" 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 | Gaia DR3 390499152406099584 | 00:39:07.86 +48:10:14.6 (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 22.1516* 00 39 07.27 +48 10 19.6 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390499152406099584,2461093.6516,13.02,0.05,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 390499152406099584 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:07.27 +48:10:19.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 19 23.91 +48 26 38.1 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
target,2461093.6516,13.27,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:19:23.91 +48:26:38.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.03 00:36:25.84 +41:03:26.3
119.88727 -21.72571 galactic And Second-epoch detections are separated by 4.3" 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 J009.1143+41.0570 | 00:36:26.45 +41:03:31.7 (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 22.1516* 00 36 25.84 +41 03 26.3 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
ATO J009.1143+41.0570,2461093.6516,13.03,0.05,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
ATO J009.1143+41.0570 20260222.1516 13.03CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:25.84 +41:03:26.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.04 00:31:05.63 +46:50:59.2
119.31787 -15.87916 galactic Cas 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 389430083506460928 | 00:31:06.37 +46:51:00.3 (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 22.1516* 00 31 05.63 +46 50 59.2 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389430083506460928,2461093.6516,13.04,0.05,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
Gaia DR3 389430083506460928 20260222.1516 13.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:05.63 +46:50:59.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.01 00:45:08.14 +46:22:02.1
121.79816 -16.49062 galactic And Second-epoch detections are separated by 7.3" 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 varaible 389778143356931712 | 00:45:08.91 +46:22:05.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 45 08.14 +46 22 02.1 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 varaible 389778143356931712,2461093.6516,13.01,0.05,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 varaible 389778143356931712 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:08.14 +46:22:02.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.99 00:45:46.38 +42:25:21.5
121.81629 -20.43684 galactic And Second-epoch detections are separated by 3.0" 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 varaible 375343827724041984 | 00:45:45.26 +42:25:23.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 45 46.38 +42 25 21.5 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 varaible 375343827724041984,2461093.6516,12.99,0.05,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 varaible 375343827724041984 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:46.38 +42:25:21.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.14 00:45:32.07 +42:27:42.3
121.77036 -20.39668 galactic And Second-epoch detections are separated by 6.4" 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 varaible 387353720217691136 | 00:45:31.58 +42:27:35.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 45 32.07 +42 27 42.3 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 varaible 387353720217691136,2461093.6516,13.14,0.05,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 varaible 387353720217691136 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:32.07 +42:27:42.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.06 00:42:59.97 +41:05:53.6
121.22049 -21.74548 galactic And Second-epoch detections are separated by 3.0" and 5.3 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 J010.7470+41.1080 | 00:42:59.85 +41:06:01.4 (Gaia DR3) | CBH (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 22.1516* 00 42 59.97 +41 05 53.6 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
ATO J010.7470+41.1080,2461093.6516,13.06,0.05,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 J010.7470+41.1080 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:59.97 +41:05:53.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.95 00:35:36.91 +43:02:35.6
119.86153 -19.73418 galactic And Second-epoch detections are separated by 6.7" 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 | Gaia DR3 varaible 381666496323483136 | 00:35:39.51 +43:03:12.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 35 36.91 +43 02 35.6 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 varaible 381666496323483136,2461093.6516,12.95,0.05,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 varaible 381666496323483136 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:36.91 +43:02:35.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.98 00:38:24.78 +44:16:41.4
120.47367 -18.53140 galactic And Second-epoch detections are separated by 6.8" 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 | ATO J009.6095+44.2781 | 00:38:26.29 +44:16:41.2 (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 22.1516* 00 38 24.78 +44 16 41.4 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
ATO J009.6095+44.2781,2461093.6516,12.98,0.05,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
ATO J009.6095+44.2781 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:24.78 +44:16:41.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.16 00:37:27.73 +42:03:43.4
120.15894 -20.73443 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 varaible 381464357983338624 | 00:37:27.98 +42:03:50.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 37 27.73 +42 03 43.4 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 varaible 381464357983338624,2461093.6516,13.16,0.05,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 varaible 381464357983338624 20260222.1516 13.16CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:27.73 +42:03:43.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.78 00:33:09.14 +42:48:18.3
119.36562 -19.94001 galactic And Second-epoch detections are separated by 3.5" 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 varaible 382389562657218816 | 00:33:09.58 +42:48:09.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 33 09.14 +42 48 18.3 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 varaible 382389562657218816,2461093.6516,12.78,0.05,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 varaible 382389562657218816 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:09.14 +42:48:18.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.94 00:36:54.15 +48:50:38.7
120.46857 -13.95813 galactic Cas 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 | Gaia DR3 391304544673642752 | 00:36:54.97 +48:50:38.1 (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 22.1516* 00 36 54.15 +48 50 38.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391304544673642752,2461093.6516,12.94,0.05,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 391304544673642752 20260222.1516 12.94CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:54.15 +48:50:38.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.01 00:38:17.33 +43:36:12.0
120.41180 -19.20406 galactic And Second-epoch detections are separated by 3.0" 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 | Gaia DR3 varaible 387657906981458560 | 00:38:17.20 +43:36:17.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 38 17.33 +43 36 12.0 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 varaible 387657906981458560,2461093.6516,13.01,0.05,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 varaible 387657906981458560 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:17.33 +43:36:12.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.87 00:35:46.84 +41:39:44.1
119.79805 -21.11421 galactic And Second-epoch detections are separated by 7.8" 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 varaible 381478071814664192 | 00:35:47.41 +41:39:48.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 35 46.84 +41 39 44.1 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 varaible 381478071814664192,2461093.6516,12.87,0.05,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 varaible 381478071814664192 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:46.84 +41:39:44.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.93 00:35:38.15 +41:02:02.2
119.72466 -21.73938 galactic And Second-epoch detections are separated by 4.7" 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 varaible 381025794577933824 | 00:35:38.67 +41:02:05.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 35 38.15 +41 02 02.2 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
Gaia DR3 varaible 381025794577933824,2461093.6516,12.93,0.05,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 varaible 381025794577933824 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:38.15 +41:02:02.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.08 00:54:44.06 +41:23:44.1
123.59623 -21.47191 galactic And Second-epoch detections are separated by 2.4" 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 | Gaia DR3 varaible 375077088778179072 | 00:54:43.96 +41:23:51.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 54 44.06 +41 23 44.1 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 varaible 375077088778179072,2461093.6516,13.08,0.05,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 varaible 375077088778179072 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:54:44.06 +41:23:44.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 38 32.84 +43 35 18.0 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 387657705119792896,2461093.6516,12.95,0.05,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 387657705119792896 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:32.84 +43:35:18.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.95 00:40:04.02 +42:13:37.6
120.68354 -20.59499 galactic And Second-epoch detections are separated by 5.1" 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 varaible 381386331319504640 | 00:40:04.44 +42:13:32.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 40 04.02 +42 13 37.6 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 varaible 381386331319504640,2461093.6516,12.95,0.05,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 varaible 381386331319504640 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:04.02 +42:13:37.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.88 00:49:57.43 +45:10:25.3
122.65799 -17.69727 galactic And Second-epoch detections are separated by 0.5" 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 | 00:49:57.43 +45:10:25.3 (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 22.1516* 00 49 57.43 +45 10 25.3 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
target,2461093.6516,12.88,0.05,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 20260222.1516 12.88CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:49:57.43 +45:10:25.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.03 00:42:19.61 +42:25:25.9
121.13801 -20.41615 galactic And Second-epoch detections are separated by 8.3" 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 | Gaia DR3 varaible 387383789285324928 | 00:42:20.09 +42:25:15.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 42 19.61 +42 25 25.9 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 varaible 387383789285324928,2461093.6516,13.03,0.05,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 varaible 387383789285324928 20260222.1516 13.03CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:19.61 +42:25:25.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.90 00:35:02.82 +42:35:09.7
119.71858 -20.18343 galactic And Second-epoch detections are separated by 3.2" 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 | Gaia DR3 varaible 381629426462661632 | 00:35:02.78 +42:35:16.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 35 02.82 +42 35 09.7 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 varaible 381629426462661632,2461093.6516,12.90,0.05,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
Gaia DR3 varaible 381629426462661632 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:02.82 +42:35:09.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.95 00:33:09.09 +42:48:22.6
119.36555 -19.93881 galactic And Second-epoch detections are separated by 5.8" and 5.3 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 varaible 382389562657218816 | 00:33:09.58 +42:48:09.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 33 09.09 +42 48 22.6 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 varaible 382389562657218816,2461093.6516,12.95,0.05,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 varaible 382389562657218816 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:09.09 +42:48:22.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.86 00:36:49.40 +44:35:15.5
120.19356 -18.20639 galactic And Second-epoch detections are separated by 6.3" 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 varaible 387857640141260288 | 00:36:49.46 +44:35:21.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 36 49.40 +44 35 15.5 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 varaible 387857640141260288,2461093.6516,12.86,0.05,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
Gaia DR3 varaible 387857640141260288 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:49.40 +44:35:15.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.97 00:37:34.52 +44:27:48.1
120.32685 -18.33826 galactic And Second-epoch detections are separated by 4.2" 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 varaible 387844347218549120 | 00:37:33.62 +44:27:55.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 37 34.52 +44 27 48.1 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 varaible 387844347218549120,2461093.6516,12.97,0.05,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 varaible 387844347218549120 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:34.52 +44:27:48.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.97 00:41:27.25 +42:12:52.2
120.95705 -20.61896 galactic And Second-epoch detections are separated by 4.7" 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 | ATO J010.3687+42.2167 | 00:41:27.58 +42:12:57.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 22.1516* 00 41 27.25 +42 12 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 J010.3687+42.2167,2461093.6516,12.97,0.05,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 J010.3687+42.2167 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:27.25 +42:12:52.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.80 00:32:54.83 +41:50:09.4
119.23992 -20.90297 galactic And Second-epoch detections are separated by 8.7" 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 varaible 381871452162391040 | 00:32:55.43 +41:50:15.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 32 54.83 +41 50 09.4 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 varaible 381871452162391040,2461093.6516,12.80,0.05,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 varaible 381871452162391040 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:54.83 +41:50:09.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.96 00:32:55.07 +40:52:22.6
119.16093 -21.86316 galactic And Second-epoch detections are separated by 5.5" 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 varaible 381055889412846976 | 00:32:54.37 +40:52:16.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 32 55.07 +40 52 22.6 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 varaible 381055889412846976,2461093.6516,12.96,0.05,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 varaible 381055889412846976 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:55.07 +40:52:22.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.92 00:35:44.15 +41:15:09.3
119.76033 -21.52245 galactic And Second-epoch detections are separated by 0.8" 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 varaible 381416460506932736 | 00:35:45.60 +41:15:13.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 35 44.15 +41 15 09.3 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 varaible 381416460506932736,2461093.6516,12.92,0.05,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 varaible 381416460506932736 20260222.1516 12.92CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:44.15 +41:15:09.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.93 00:40:38.56 +43:06:25.1
120.83911 -19.72091 galactic And Second-epoch detections are separated by 1.7" 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 varaible 387440615997583104 | 00:40:38.95 +43:06:30.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 40 38.56 +43 06 25.1 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 varaible 387440615997583104,2461093.6516,12.93,0.05,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 varaible 387440615997583104 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:38.56 +43:06:25.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.09 00:43:11.12 +41:36:14.9
121.27688 -21.24109 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 | Gaia DR3 varaible 381298709684828928 | 00:43:11.49 +41:36:19.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: M0 (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 22.1516* 00 43 11.12 +41 36 14.9 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 varaible 381298709684828928,2461093.6516,13.09,0.05,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 varaible 381298709684828928 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:11.12 +41:36:14.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.79 00:33:27.98 +44:19:03.1
119.54494 -18.43600 galactic And Second-epoch detections are separated by 4.4" 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 | Gaia DR3 varaible 388498380541664640 | 00:33:28.76 +44:18:55.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 33 27.98 +44 19 03.1 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 varaible 388498380541664640,2461093.6516,12.79,0.05,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 varaible 388498380541664640 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:27.98 +44:19:03.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.07 01:10:43.33 +43:20:57.2
126.64658 -19.38339 galactic And Second-epoch detections are separated by 4.8" 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 | target | 01:10:43.33 +43:20:57.2 (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 22.1516* 01 10 43.33 +43 20 57.2 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
target,2461093.6516,13.07,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:10:43.33 +43:20:57.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.80 00:45:35.47 +43:34:46.5
121.81018 -19.27943 galactic And Second-epoch detections are separated by 6.0" 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 | target | 00:45:35.47 +43:34:46.5 (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 22.1516* 00 45 35.47 +43 34 46.5 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
target,2461093.6516,12.80,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:35.47 +43:34:46.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.79 00:44:52.33 +41:25:03.3
121.60957 -21.43731 galactic And Second-epoch detections are separated by 5.0" 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 varaible 369280536494597248 | 00:44:52.74 +41:25:10.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 44 52.33 +41 25 03.3 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 varaible 369280536494597248,2461093.6516,12.79,0.05,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 varaible 369280536494597248 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:52.33 +41:25:03.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.78 00:37:48.84 +43:51:08.4
120.33565 -18.95073 galactic And Second-epoch detections are separated by 4.6" 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 | Gaia DR3 varaible 387802458400805120 | 00:37:48.98 +43:51:14.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 37 48.84 +43 51 08.4 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 varaible 387802458400805120,2461093.6516,12.78,0.05,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 varaible 387802458400805120 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:48.84 +43:51:08.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.89 00:35:00.04 +42:13:42.7
119.68358 -20.53952 galactic And Second-epoch detections are separated by 2.4" 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 | ATO J008.7481+42.2356 | 00:35:00.39 +42:13:34.2 (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 22.1516* 00 35 00.04 +42 13 42.7 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 J008.7481+42.2356,2461093.6516,12.89,0.05,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 J008.7481+42.2356 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:00.04 +42:13:42.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.93 00:36:28.24 +44:27:45.7
120.11953 -18.32731 galactic And Second-epoch detections are separated by 5.6" 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 J009.1140+44.4611 | 00:36:27.87 +44:27:51.8 (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 22.1516* 00 36 28.24 +44 27 45.7 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 J009.1140+44.4611,2461093.6516,12.93,0.05,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
ATO J009.1140+44.4611 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:28.24 +44:27:45.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.96 00:40:45.58 +42:16:48.8
120.82290 -20.54779 galactic And Second-epoch detections are separated by 8.0" and 5.0 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 varaible 381390935527691008 | 00:40:46.22 +42:16:53.4 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 40 45.58 +42 16 48.8 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 varaible 381390935527691008,2461093.6516,12.96,0.05,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 varaible 381390935527691008 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:45.58 +42:16:48.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.72 00:29:04.68 +46:31:28.9
118.93039 -16.17325 galactic And Second-epoch detections are separated by 3.1" 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 | ATO J007.2672+46.5266 | 00:29:05.44 +46:31:33.5 (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 22.1516* 00 29 04.68 +46 31 28.9 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
ATO J007.2672+46.5266,2461093.6516,12.72,0.05,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
ATO J007.2672+46.5266 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:04.68 +46:31:28.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.81 00:46:37.44 +41:08:56.1
121.95651 -21.71371 galactic And 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 | ATO J011.6518+41.1570 | 00:46:37.13 +41:08:44.4 (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 22.1516* 00 46 37.44 +41 08 56.1 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
ATO J011.6518+41.1570,2461093.6516,12.81,0.05,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
ATO J011.6518+41.1570 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:37.44 +41:08:56.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.89 00:44:53.46 +49:53:06.5
121.84980 -12.97285 galactic Cas Second-epoch detections are separated by 3.0" 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 414677237002943360 | 00:44:54.01 +49:53:09.1 (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 22.1516* 00 44 53.46 +49 53 06.5 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414677237002943360,2461093.6516,12.89,0.05,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 414677237002943360 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:53.46 +49:53:06.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.82 00:43:00.26 +41:28:54.6
121.23599 -21.36214 galactic And Second-epoch detections are separated by 0.5" 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 varaible 381273871896232448 | 00:43:00.75 +41:28:57.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 43 00.26 +41 28 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
Gaia DR3 varaible 381273871896232448,2461093.6516,12.82,0.05,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 varaible 381273871896232448 20260222.1516 12.82CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:00.26 +41:28:54.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.78 00:31:24.11 +44:25:24.4
119.16603 -18.30175 galactic And Second-epoch detections are separated by 6.2" and 5.3 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 varaible 388547106947790464 | 00:31:24.52 +44:25:32.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 31 24.11 +44 25 24.4 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 varaible 388547106947790464,2461093.6516,12.78,0.05,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 varaible 388547106947790464 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:24.11 +44:25:24.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.74 00:42:30.39 +44:32:12.6
121.25569 -18.30584 galactic And Second-epoch detections are separated by 3.0" 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 | Gaia DR3 varaible 387997587354952832 | 00:42:29.81 +44:32:03.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 42 30.39 +44 32 12.6 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 varaible 387997587354952832,2461093.6516,12.74,0.05,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 varaible 387997587354952832 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:30.39 +44:32:12.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.91 00:41:21.83 +46:23:45.3
121.12120 -16.44041 galactic And Second-epoch detections are separated by 5.3" and 4.6 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 varaible 389873113673972608 | 00:41:20.74 +46:23:44.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 41 21.83 +46 23 45.3 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 varaible 389873113673972608,2461093.6516,12.91,0.05,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
Gaia DR3 varaible 389873113673972608 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:21.83 +46:23:45.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.69 00:39:41.74 +41:26:54.8
120.56949 -21.36932 galactic And Second-epoch detections are separated by 5.4" 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 varaible 381237622366596992 | 00:39:42.79 +41:26:55.4 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 39 41.74 +41 26 54.8 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 varaible 381237622366596992,2461093.6516,12.69,0.05,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 varaible 381237622366596992 20260222.1516 12.69CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:41.74 +41:26:54.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.74 00:32:54.29 +47:07:43.0
119.66047 -15.62538 galactic Cas Second-epoch detections are separated by 4.5" 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 389273849775366528 | 00:32:54.91 +47:07:36.1 (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 22.1516* 00 32 54.29 +47 07 43.0 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389273849775366528,2461093.6516,12.74,0.05,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 389273849775366528 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:54.29 +47:07:43.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.70 00:27:31.57 +48:49:15.5
118.88186 -13.86265 galactic Cas Second-epoch detections are separated by 7.7" 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 391198304358400512 | 00:27:32.06 +48:49:10.3 (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 22.1516* 00 27 31.57 +48 49 15.5 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391198304358400512,2461093.6516,12.70,0.05,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 391198304358400512 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:31.57 +48:49:15.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.72 00:42:24.39 +43:09:57.8
121.18317 -19.67503 galactic And Second-epoch detections are separated by 7.1" 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 varaible 387525484549784064 | 00:42:25.07 +43:10:08.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 42 24.39 +43 09 57.8 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 varaible 387525484549784064,2461093.6516,12.72,0.05,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 varaible 387525484549784064 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:24.39 +43:09:57.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.90 00:55:13.37 +46:39:01.7
123.60835 -16.21631 galactic And Second-epoch detections are separated by 6.1" 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 378069207813123456 | 00:55:12.24 +46:38:58.3 (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 22.1516* 00 55 13.37 +46 39 01.7 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 378069207813123456,2461093.6516,12.90,0.05,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
Gaia DR3 378069207813123456 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:55:13.37 +46:39:01.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.73 00:47:20.19 +43:53:19.0
122.15050 -18.97691 galactic And Second-epoch detections are separated by 1.3" 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 varaible 375899355973076096 | 00:47:20.34 +43:53:24.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 47 20.19 +43 53 19.0 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 varaible 375899355973076096,2461093.6516,12.73,0.05,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 varaible 375899355973076096 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:47:20.19 +43:53:19.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.60 00:33:35.66 +45:30:31.1
119.66001 -17.24972 galactic And Second-epoch detections are separated by 8.2" 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 varaible 389024329352952320 | 00:33:36.61 +45:30:32.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 33 35.66 +45 30 31.1 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
Gaia DR3 varaible 389024329352952320,2461093.6516,12.60,0.05,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
Gaia DR3 varaible 389024329352952320 20260222.1516 12.60CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:35.66 +45:30:31.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 11 14.09 +50 23 29.3 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 403528841933317632,2461093.6516,12.97,0.05,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 403528841933317632 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:11:14.09 +50:23:29.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.79 00:35:45.77 +49:23:12.7
120.31068 -13.40509 galactic Cas Second-epoch detections are separated by 4.3" 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 | ATO J008.9313+49.3830 | 00:35:46.42 +49:23:13.2 (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 22.1516* 00 35 45.77 +49 23 12.7 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J008.9313+49.3830,2461093.6516,12.79,0.05,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 J008.9313+49.3830 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:45.77 +49:23:12.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.88 00:44:08.79 +42:27:38.3
121.49731 -20.39080 galactic And Second-epoch detections are separated by 3.0" 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 varaible 387351147534006016 | 00:44:09.93 +42:27:38.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 44 08.79 +42 27 38.3 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 varaible 387351147534006016,2461093.6516,12.88,0.05,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 varaible 387351147534006016 20260222.1516 12.88CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:08.79 +42:27:38.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.83 00:40:42.40 +48:48:37.5
121.11123 -14.02339 galactic Cas Second-epoch detections are separated by 3.5" 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 | Gaia DR3 390635079530793600 | 00:40:42.48 +48:48:29.3 (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 22.1516* 00 40 42.40 +48 48 37.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390635079530793600,2461093.6516,12.83,0.05,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 390635079530793600 20260222.1516 12.83CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:42.40 +48:48:37.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.77 00:33:28.11 +42:03:50.7
119.36840 -20.68330 galactic And Second-epoch detections are separated by 7.7" 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 varaible 382247042759156864 | 00:33:28.70 +42:03:43.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 33 28.11 +42 03 50.7 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 varaible 382247042759156864,2461093.6516,12.77,0.05,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 varaible 382247042759156864 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:28.11 +42:03:50.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.78 00:38:45.74 +43:49:49.7
120.51496 -18.98178 galactic And Second-epoch detections are separated by 2.5" 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 varaible 387756004034532224 | 00:38:46.15 +43:49:58.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 38 45.74 +43 49 49.7 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 varaible 387756004034532224,2461093.6516,12.78,0.05,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 varaible 387756004034532224 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:45.74 +43:49:49.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.84 00:42:52.87 +43:18:59.8
121.28067 -19.52770 galactic And Second-epoch detections are separated by 4.0" and 5.3 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 varaible 387530982107920256 | 00:42:53.40 +43:19:02.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 42 52.87 +43 18 59.8 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 varaible 387530982107920256,2461093.6516,12.84,0.05,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 varaible 387530982107920256 20260222.1516 12.84CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:52.87 +43:18:59.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.79 00:40:46.85 +50:18:46.7
121.18943 -12.52272 galactic Cas Second-epoch detections are separated by 3.6" and 5.1 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 414750908580993408 | 00:40:47.00 +50:18:56.5 (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 22.1516* 00 40 46.85 +50 18 46.7 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414750908580993408,2461093.6516,12.79,0.05,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 414750908580993408 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:46.85 +50:18:46.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.64 00:39:18.67 +48:30:25.9
120.85949 -14.31575 galactic Cas Second-epoch detections are separated by 6.5" 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 390533821382028416 | 00:39:19.36 +48:30:34.9 (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 22.1516* 00 39 18.67 +48 30 25.9 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390533821382028416,2461093.6516,12.64,0.05,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 390533821382028416 20260222.1516 12.64CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:18.67 +48:30:25.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.75 00:38:48.42 +46:30:21.2
120.66793 -16.31033 galactic And Second-epoch detections are separated by 5.3" 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 varaible 389921427764072704 | 00:38:49.27 +46:30:24.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 38 48.42 +46 30 21.2 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 varaible 389921427764072704,2461093.6516,12.75,0.05,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 varaible 389921427764072704 20260222.1516 12.75CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:48.42 +46:30:21.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.57 00:30:50.61 +43:43:00.9
118.99854 -18.99749 galactic And Second-epoch detections are separated by 5.6" 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 varaible 382497422172695296 | 00:30:50.83 +43:42:51.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 30 50.61 +43 43 00.9 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 varaible 382497422172695296,2461093.6516,12.57,0.05,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 varaible 382497422172695296 20260222.1516 12.57CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:50.61 +43:43:00.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.78 00:36:22.78 +50:38:17.7
120.49058 -12.16211 galactic Cas Second-epoch detections are separated by 5.9" and 5.3 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 415567433403070848 | 00:36:23.45 +50:38:13.7 (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 22.1516* 00 36 22.78 +50 38 17.7 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415567433403070848,2461093.6516,12.78,0.05,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 415567433403070848 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:22.78 +50:38:17.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.11 01:07:07.67 +43:02:44.6
125.97640 -19.73326 galactic And Second-epoch detections are separated by 1.6" 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 | ATO J016.7848+43.0429 | 01:07:08.37 +43:02:34.4 (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 22.1516* 01 07 07.67 +43 02 44.6 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
ATO J016.7848+43.0429,2461093.6516,13.11,0.05,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
ATO J016.7848+43.0429 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:07:07.67 +43:02:44.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.94 00:51:35.56 +41:37:04.6
122.96295 -21.25379 galactic And 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 | Gaia DR3 varaible 375141513288414848 | 00:51:34.99 +41:37:12.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: K5 (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 22.1516* 00 51 35.56 +41 37 04.6 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 varaible 375141513288414848,2461093.6516,12.94,0.05,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 varaible 375141513288414848 20260222.1516 12.94CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:51:35.56 +41:37:04.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 36 34.59 +49 09 03.9 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391317979331254144,2461093.6516,12.64,0.05,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 391317979331254144 20260222.1516 12.64CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:34.59 +49:09:03.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.63 00:27:53.38 +46:08:08.5
118.67992 -16.54155 galactic And Second-epoch detections are separated by 6.8" 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 | Gaia DR3 388927705473478016 | 00:27:54.20 +46:08:01.3 (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 22.1516* 00 27 53.38 +46 08 08.5 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 388927705473478016,2461093.6516,12.63,0.05,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
Gaia DR3 388927705473478016 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:53.38 +46:08:08.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.74 00:37:30.07 +45:50:30.3
120.39504 -16.96134 galactic And Second-epoch detections are separated by 5.4" 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 | Gaia DR3 varaible 388386917550418816 | 00:37:29.39 +45:50:42.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 37 30.07 +45 50 30.3 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 varaible 388386917550418816,2461093.6516,12.74,0.05,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 varaible 388386917550418816 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:30.07 +45:50:30.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.93 00:55:48.81 +44:10:48.4
123.76003 -18.68460 galactic And Second-epoch detections are separated by 4.1" 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 varaible 377258279329641728 | 00:55:47.20 +44:10:53.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 55 48.81 +44 10 48.4 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 varaible 377258279329641728,2461093.6516,12.93,0.05,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 varaible 377258279329641728 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:55:48.81 +44:10:48.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.61 00:29:05.57 +45:41:25.8
118.85435 -17.00426 galactic And Second-epoch detections are separated by 2.1" 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 | Gaia DR3 varaible 388900874815157504 | 00:29:03.85 +45:41:29.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 29 05.57 +45 41 25.8 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 varaible 388900874815157504,2461093.6516,12.61,0.05,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 varaible 388900874815157504 20260222.1516 12.61CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:05.57 +45:41:25.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.72 00:35:25.34 +49:55:43.8
120.28935 -12.86072 galactic Cas Second-epoch detections are separated by 0.9" 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 391502624266678784 | 00:35:25.41 +49:55:36.9 (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 22.1516* 00 35 25.34 +49 55 43.8 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391502624266678784,2461093.6516,12.72,0.05,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 391502624266678784 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:25.34 +49:55:43.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.65 00:36:29.53 +49:32:09.7
120.44161 -13.26344 galactic Cas Second-epoch detections are separated by 2.7" 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 391470261691517440 | 00:36:30.23 +49:32:06.8 (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 22.1516* 00 36 29.53 +49 32 09.7 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391470261691517440,2461093.6516,12.65,0.05,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 391470261691517440 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:29.53 +49:32:09.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 40 55.67 +40 57 43.4 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 381160725272239744,2461093.6516,12.90,0.05,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
Gaia DR3 381160725272239744 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:55.67 +40:57:43.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.76 00:41:18.74 +44:10:21.0
121.01580 -18.66157 galactic And Second-epoch detections are separated by 8.3" and 4.5 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 varaible 387590871132454912 | 00:41:19.50 +44:10:13.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 41 18.74 +44 10 21.0 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 varaible 387590871132454912,2461093.6516,12.76,0.05,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 varaible 387590871132454912 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:18.74 +44:10:21.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.80 00:34:28.88 +42:30:06.4
119.60162 -20.26030 galactic And Second-epoch detections are separated by 2.6" 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 varaible 381538441873070976 | 00:34:28.11 +42:30:04.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 34 28.88 +42 30 06.4 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 varaible 381538441873070976,2461093.6516,12.80,0.05,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 varaible 381538441873070976 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:28.88 +42:30:06.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.62 00:51:55.88 +51:02:22.0
123.01116 -11.83223 galactic Cas Second-epoch detections are separated by 2.5" 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 | ATO J012.9851+51.0299 | 00:51:55.68 +51:02:15.5 (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 22.1516* 00 51 55.88 +51 02 22.0 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J012.9851+51.0299,2461093.6516,12.62,0.05,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
ATO J012.9851+51.0299 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:51:55.88 +51:02:22.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.64 00:33:59.04 +50:30:22.6
120.09349 -12.26925 galactic Cas Second-epoch detections are separated by 4.6" and 5.1 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 415738579260650240 | 00:33:56.42 +50:30:03.5 (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 22.1516* 00 33 59.04 +50 30 22.6 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415738579260650240,2461093.6516,12.64,0.05,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 415738579260650240 20260222.1516 12.64CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:59.04 +50:30:22.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.74 00:43:25.55 +41:24:23.1
121.31800 -21.44022 galactic And Second-epoch detections are separated by 4.2" 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 J010.8626+41.4095 | 00:43:26.21 +41:24:46.2 (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 22.1516* 00 43 25.55 +41 24 23.1 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
ATO J010.8626+41.4095,2461093.6516,12.74,0.05,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 J010.8626+41.4095 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:25.55 +41:24:23.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 28 39.06 +46 42 07.2 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
T-Cas0-01550,2461093.6516,12.54,0.05,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
T-Cas0-01550 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:39.06 +46:42:07.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.64 00:46:38.86 +42:57:47.0
121.99992 -19.90002 galactic And Second-epoch detections are separated by 4.2" 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 J011.6635+42.9649 | 00:46:38.86 +42:57:47.0 (user input) | dubious (ATLAS) | (ATLAS) | (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 22.1516* 00 46 38.86 +42 57 47.0 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
ATO J011.6635+42.9649,2461093.6516,12.64,0.05,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
ATO J011.6635+42.9649 20260222.1516 12.64CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:38.86 +42:57:47.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 33 55.78 +46 08 48.1 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
Gaia DR3 389068653417199616,2461093.6516,12.62,0.05,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 389068653417199616 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:55.78 +46:08:48.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 36 00.05 +46 04 24.3 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
NSVS 3737167,2461093.6516,12.70,0.05,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
NSVS 3737167 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:00.05 +46:04:24.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.73 00:38:51.55 +43:44:31.9
120.52858 -19.07085 galactic And Second-epoch detections are separated by 3.6" 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 varaible 387751296750378624 | 00:38:51.03 +43:44:24.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 38 51.55 +43 44 31.9 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 varaible 387751296750378624,2461093.6516,12.73,0.05,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 varaible 387751296750378624 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:51.55 +43:44:31.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.81 00:45:30.88 +40:58:40.2
121.72722 -21.88006 galactic And Second-epoch detections are separated by 1.5" 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 varaible 369212160615317504 | 00:45:31.75 +40:58:56.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 45 30.88 +40 58 40.2 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 varaible 369212160615317504,2461093.6516,12.81,0.05,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 varaible 369212160615317504 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:30.88 +40:58:40.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 42 11.80 +48 53 19.9 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390628310662325760,2461093.6516,12.58,0.05,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 390628310662325760 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:11.80 +48:53:19.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.64 00:30:44.42 +47:48:53.3
119.33858 -14.91248 galactic Cas Second-epoch detections are separated by 8.3" 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 390984513772212736 | 00:30:45.17 +47:48:49.0 (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 22.1516* 00 30 44.42 +47 48 53.3 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390984513772212736,2461093.6516,12.64,0.05,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 390984513772212736 20260222.1516 12.64CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:44.42 +47:48:53.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.59 00:39:02.12 +49:30:32.7
120.86354 -13.31285 galactic Cas Second-epoch detections are separated by 7.1" 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 391429785919972992 | 00:39:01.29 +49:30:18.7 (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 22.1516* 00 39 02.12 +49 30 32.7 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391429785919972992,2461093.6516,12.59,0.05,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 391429785919972992 20260222.1516 12.59CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:02.12 +49:30:32.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.68 00:34:35.69 +47:34:42.4
119.98984 -15.19707 galactic Cas Second-epoch detections are separated by 3.5" 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 | Gaia DR3 390796054905467008 | 00:34:36.56 +47:34:39.6 (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 22.1516* 00 34 35.69 +47 34 42.4 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390796054905467008,2461093.6516,12.68,0.05,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 390796054905467008 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:35.69 +47:34:42.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.80 00:49:36.89 +41:29:06.4
122.56524 -21.38534 galactic And Second-epoch detections are separated by 4.8" 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 varaible 375054312567767040 | 00:49:37.67 +41:29:16.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 49 36.89 +41 29 06.4 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 varaible 375054312567767040,2461093.6516,12.80,0.05,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 varaible 375054312567767040 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:49:36.89 +41:29:06.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.54 00:32:50.08 +42:34:54.4
119.28556 -20.15822 galactic And Second-epoch detections are separated by 4.2" 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 varaible 382298582366655360 | 00:32:49.24 +42:34:54.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 32 50.08 +42 34 54.4 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
Gaia DR3 varaible 382298582366655360,2461093.6516,12.54,0.05,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
Gaia DR3 varaible 382298582366655360 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:50.08 +42:34:54.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 39 25.42 +47 25 28.8 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390080960030502272,2461093.6516,12.55,0.05,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 390080960030502272 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:25.42 +47:25:28.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.47 00:34:42.75 +43:33:40.6
119.72453 -19.20629 galactic And Second-epoch detections are separated by 2.6" 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 varaible 388437980419008512 | 00:34:42.05 +43:33:34.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 34 42.75 +43 33 40.6 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 varaible 388437980419008512,2461093.6516,12.47,0.05,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 varaible 388437980419008512 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:42.75 +43:33:40.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.62 00:37:33.86 +41:55:06.5
120.17034 -20.87887 galactic And Second-epoch detections are separated by 4.9" 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 | Gaia DR3 varaible 381461476060527488 | 00:37:33.62 +41:55:01.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 37 33.86 +41 55 06.5 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 varaible 381461476060527488,2461093.6516,12.62,0.05,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 varaible 381461476060527488 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:33.86 +41:55:06.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.51 00:32:04.48 +43:46:41.9
119.23819 -18.95453 galactic And Second-epoch detections are separated by 0.2" 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 | Gaia DR3 varaible 382500926866751744 | 00:32:04.05 +43:46:35.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 32 04.48 +43 46 41.9 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
Gaia DR3 varaible 382500926866751744,2461093.6516,12.51,0.05,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 varaible 382500926866751744 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:04.48 +43:46:41.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.54 00:36:05.33 +44:20:32.8
120.03995 -18.44310 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 varaible 387833042864539904 | 00:36:05.10 +44:20:23.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 36 05.33 +44 20 32.8 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 varaible 387833042864539904,2461093.6516,12.54,0.05,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
Gaia DR3 varaible 387833042864539904 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:05.33 +44:20:32.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.70 00:52:35.41 +44:54:12.9
123.14641 -17.96769 galactic And Second-epoch detections are separated by 5.0" 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 varaible 377501271399073920 | 00:52:35.53 +44:54:28.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 52 35.41 +44 54 12.9 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 varaible 377501271399073920,2461093.6516,12.70,0.05,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 varaible 377501271399073920 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:52:35.41 +44:54:12.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.48 00:35:45.81 +42:25:30.9
119.84768 -20.35261 galactic And Second-epoch detections are separated by 6.5" 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 varaible 381615648206872960 | 00:35:45.00 +42:25:32.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 35 45.81 +42 25 30.9 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
Gaia DR3 varaible 381615648206872960,2461093.6516,12.48,0.05,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 varaible 381615648206872960 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:45.81 +42:25:30.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.61 00:30:30.05 +44:28:06.2
119.00124 -18.24351 galactic And Second-epoch detections are separated by 4.9" 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 varaible 388536558506190464 | 00:30:29.17 +44:28:05.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 30 30.05 +44 28 06.2 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 varaible 388536558506190464,2461093.6516,12.61,0.05,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 varaible 388536558506190464 20260222.1516 12.61CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:30.05 +44:28:06.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.47 00:38:46.51 +46:52:37.6
120.68201 -15.93931 galactic Cas Second-epoch detections are separated by 8.4" and 4.2 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 389966954418214272 | 00:38:47.07 +46:52:40.8 (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 22.1516* 00 38 46.51 +46 52 37.6 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389966954418214272,2461093.6516,12.47,0.05,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 389966954418214272 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:46.51 +46:52:37.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 03 40.80 +48 10 46.9 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
target,2461093.6516,12.60,0.05,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 20260222.1516 12.60CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:03:40.80 +48:10:46.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 47 55.32 +49 51 36.5 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414570554314127104,2461093.6516,12.63,0.05,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
Gaia DR3 414570554314127104 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:47:55.32 +49:51:36.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.54 00:40:03.46 +41:19:01.0
120.63554 -21.50406 galactic And Second-epoch detections are separated by 7.5" and 4.4 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 varaible 381233121240894848 | 00:40:04.30 +41:19:07.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 40 03.46 +41 19 01.0 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 varaible 381233121240894848,2461093.6516,12.54,0.05,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
Gaia DR3 varaible 381233121240894848 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:03.46 +41:19:01.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.42 00:33:39.87 +44:07:45.0
119.56775 -18.62645 galactic And Second-epoch detections are separated by 8.3" 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 varaible 388489240851270272 | 00:33:40.29 +44:07:34.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 33 39.87 +44 07 45.0 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 varaible 388489240851270272,2461093.6516,12.42,0.05,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 varaible 388489240851270272 20260222.1516 12.42CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:39.87 +44:07:45.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.41 00:46:17.98 +50:52:33.5
122.10333 -11.98751 galactic Cas Second-epoch detections are separated by 5.1" 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 | ATO J011.5756+50.8833 | 00:46:18.20 +50:52:21.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.904+/- (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 22.1516* 00 46 17.98 +50 52 33.5 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J011.5756+50.8833,2461093.6516,12.41,0.05,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 J011.5756+50.8833 20260222.1516 12.41CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:17.98 +50:52:33.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.47 00:27:54.37 +49:29:44.4
119.01111 -13.19685 galactic Cas Second-epoch detections are separated by 0.9" 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 391244071533257216 | 00:27:54.12 +49:29:35.0 (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 22.1516* 00 27 54.37 +49 29 44.4 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391244071533257216,2461093.6516,12.47,0.05,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 391244071533257216 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:54.37 +49:29:44.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 36 36.31 +41 42 11.7 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
WISE J003635.9+414206,2461093.6516,12.77,0.05,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
WISE J003635.9+414206 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:36.31 +41:42:11.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.27 00:39:40.36 +42:36:07.8
120.62515 -20.21688 galactic And Second-epoch detections are separated by 2.3" 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 varaible 381586030112520064 | 00:39:41.61 +42:36:04.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 39 40.36 +42 36 07.8 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 varaible 381586030112520064,2461093.6516,12.27,0.05,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 varaible 381586030112520064 20260222.1516 12.27CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:40.36 +42:36:07.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.46 00:34:59.13 +43:38:26.1
119.78246 -19.13053 galactic And Second-epoch detections are separated by 2.8" 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 varaible 388444405690078336 | 00:34:59.67 +43:38:20.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 34 59.13 +43 38 26.1 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 varaible 388444405690078336,2461093.6516,12.46,0.05,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 varaible 388444405690078336 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:59.13 +43:38:26.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 13 46.30 +46 34 07.8 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 401008731219573504,2461093.6516,12.79,0.05,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 401008731219573504 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:13:46.30 +46:34:07.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.43 00:37:41.55 +47:58:23.2
120.55276 -14.83513 galactic Cas Second-epoch detections are separated by 2.8" 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 390867007765424256 | 00:37:42.30 +47:58:25.0 (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 22.1516* 00 37 41.55 +47 58 23.2 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390867007765424256,2461093.6516,12.43,0.05,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 390867007765424256 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:41.55 +47:58:23.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.54 00:47:49.56 +48:00:39.9
122.30696 -14.85628 galactic Cas Second-epoch detections are separated by 0.6" 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 390344636661482496 | 00:47:48.91 +48:00:39.8 (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 22.1516* 00 47 49.56 +48 00 39.9 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390344636661482496,2461093.6516,12.54,0.05,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
Gaia DR3 390344636661482496 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:47:49.56 +48:00:39.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.34 00:37:40.43 +46:38:53.5
120.47332 -16.15784 galactic And Second-epoch detections are separated by 7.9" 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 varaible 389938538913744128 | 00:37:38.92 +46:38:41.4 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 37 40.43 +46 38 53.5 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 varaible 389938538913744128,2461093.6516,12.34,0.05,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 varaible 389938538913744128 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:40.43 +46:38:53.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.47 00:28:53.47 +44:15:58.5
118.68047 -18.41930 galactic And Second-epoch detections are separated by 3.1" 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 varaible 382713441849513856 | 00:28:52.71 +44:15:56.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 28 53.47 +44 15 58.5 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 varaible 382713441849513856,2461093.6516,12.47,0.05,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 varaible 382713441849513856 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:53.47 +44:15:58.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 05 51.98 +48 50 26.6 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 401804296601315456,2461093.6516,12.61,0.05,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 401804296601315456 20260222.1516 12.61CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:05:51.98 +48:50:26.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 34 14.62 +42 15 49.1 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 381528202672271616,2461093.6516,12.49,0.05,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 381528202672271616 20260222.1516 12.49CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:14.62 +42:15:49.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.46 00:36:01.03 +41:23:26.6
119.82659 -21.38803 galactic And Second-epoch detections are separated by 5.8" 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 varaible 381419557179638784 | 00:36:00.54 +41:23:23.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 36 01.03 +41 23 26.6 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 varaible 381419557179638784,2461093.6516,12.46,0.05,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 varaible 381419557179638784 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:01.03 +41:23:26.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.41 00:44:50.41 +41:06:08.0
121.59378 -21.75238 galactic And Second-epoch detections are separated by 8.3" 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 varaible 369261295041164032 | 00:44:51.33 +41:06:22.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 44 50.41 +41 06 08.0 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 varaible 369261295041164032,2461093.6516,12.41,0.05,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 varaible 369261295041164032 20260222.1516 12.41CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:50.41 +41:06:08.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.44 00:32:14.76 +43:02:06.8
119.20867 -19.69774 galactic And Second-epoch detections are separated by 3.9" 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 varaible 382406746823342976 | 00:32:14.06 +43:01:56.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 32 14.76 +43 02 06.8 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 varaible 382406746823342976,2461093.6516,12.44,0.05,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 varaible 382406746823342976 20260222.1516 12.44CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:14.76 +43:02:06.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 32 58.65 +43 15 23.0 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 382436880313863040,2461093.6516,12.32,0.05,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 382436880313863040 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:58.65 +43:15:23.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.55 01:02:24.96 +47:26:32.9
124.85676 -15.38824 galactic And Second-epoch detections are separated by 6.4" 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 401997604490429312 | 01:02:23.28 +47:27:12.9 (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 22.1516* 01 02 24.96 +47 26 32.9 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 401997604490429312,2461093.6516,12.55,0.05,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 401997604490429312 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:02:24.96 +47:26:32.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.56 00:43:47.17 +44:05:58.5
121.48130 -18.75061 galactic And Second-epoch detections are separated by 4.6" 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 varaible 387952198141338880 | 00:43:48.10 +44:05:46.4 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 43 47.17 +44 05 58.5 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 varaible 387952198141338880,2461093.6516,12.56,0.05,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 varaible 387952198141338880 20260222.1516 12.56CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:47.17 +44:05:58.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.59 01:09:27.78 +42:40:17.6
126.45811 -20.07675 galactic And Second-epoch detections are separated by 5.3" 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 varaible 373187273104190976 | 01:09:26.78 +42:40:18.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 01 09 27.78 +42 40 17.6 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 varaible 373187273104190976,2461093.6516,12.59,0.05,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 varaible 373187273104190976 20260222.1516 12.59CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:09:27.78 +42:40:17.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.30 00:31:22.40 +43:13:28.5
119.05646 -19.49613 galactic And Second-epoch detections are separated by 1.3" 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 | ATO J007.8439+43.2130 | 00:31:21.51 +43:13:18.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 22.1516* 00 31 22.40 +43 13 28.5 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
ATO J007.8439+43.2130,2461093.6516,12.30,0.05,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
ATO J007.8439+43.2130 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:22.40 +43:13:28.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.44 00:29:58.05 +41:56:50.4
118.66519 -20.74647 galactic And Second-epoch detections are separated by 5.8" 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 varaible 381908358817807360 | 00:29:57.17 +41:56:45.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 29 58.05 +41 56 50.4 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 varaible 381908358817807360,2461093.6516,12.44,0.05,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 varaible 381908358817807360 20260222.1516 12.44CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:58.05 +41:56:50.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.24 00:29:26.96 +42:33:03.3
118.62119 -20.13671 galactic And Second-epoch detections are separated by 3.8" 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 varaible 382332735946324480 | 00:29:27.72 +42:33:03.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 29 26.96 +42 33 03.3 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 varaible 382332735946324480,2461093.6516,12.24,0.05,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 varaible 382332735946324480 20260222.1516 12.24CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:26.96 +42:33:03.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.15 00:33:45.26 +46:31:47.2
119.76568 -16.23323 galactic And Second-epoch detections are separated by 8.8" 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 J008.4377+46.5213 | 00:33:45.94 +46:31:53.1 (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 22.1516* 00 33 45.26 +46 31 47.2 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
ATO J008.4377+46.5213,2461093.6516,12.15,0.05,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
ATO J008.4377+46.5213 20260222.1516 12.15CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:45.26 +46:31:47.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.49 00:51:14.82 +41:02:16.8
122.89313 -21.83373 galactic And Second-epoch detections are separated by 6.8" 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 varaible 374984115622349056 | 00:51:15.28 +41:02:21.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 51 14.82 +41 02 16.8 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 varaible 374984115622349056,2461093.6516,12.49,0.05,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 varaible 374984115622349056 20260222.1516 12.49CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:51:14.82 +41:02:16.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.08 00:45:09.49 +48:17:57.1
121.85295 -14.55940 galactic Cas Second-epoch detections are separated by 4.9" 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 390361610371955968 | 00:45:09.98 +48:17:51.1 (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 22.1516* 00 45 09.49 +48 17 57.1 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390361610371955968,2461093.6516,12.08,0.05,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 390361610371955968 20260222.1516 12.08CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:45:09.49 +48:17:57.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.07 00:33:58.45 +42:07:29.3
119.47315 -20.62963 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 | ATO J008.4944+42.1318 | 00:33:57.55 +42:07:22.8 (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 22.1516* 00 33 58.45 +42 07 29.3 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
ATO J008.4944+42.1318,2461093.6516,12.07,0.05,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
ATO J008.4944+42.1318 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:58.45 +42:07:29.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.04 00:40:42.06 +48:34:27.0
121.09980 -14.25938 galactic Cas 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 390526468398201856 | 00:40:41.29 +48:34:22.8 (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 22.1516* 00 40 42.06 +48 34 27.0 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390526468398201856,2461093.6516,12.04,0.05,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
Gaia DR3 390526468398201856 20260222.1516 12.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:42.06 +48:34:27.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.14 00:41:47.58 +42:40:34.2
121.04371 -20.16022 galactic And Second-epoch detections are separated by 7.2" 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 varaible 387396433668971008 | 00:41:48.06 +42:40:39.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 41 47.58 +42 40 34.2 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 varaible 387396433668971008,2461093.6516,12.14,0.05,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 varaible 387396433668971008 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:47.58 +42:40:34.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.06 00:38:31.88 +41:33:57.7
120.34230 -21.24082 galactic And Second-epoch detections are separated by 8.1" and 5.1 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 varaible 381248853706750464 | 00:38:32.83 +41:34:10.4 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 38 31.88 +41 33 57.7 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 varaible 381248853706750464,2461093.6516,12.06,0.05,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 varaible 381248853706750464 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:31.88 +41:33:57.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.08 00:46:54.07 +49:11:17.1
122.16903 -13.67695 galactic Cas Second-epoch detections are separated by 1.2" and 5.3 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 414435108224304896 | 00:46:55.16 +49:11:14.7 (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 22.1516* 00 46 54.07 +49 11 17.1 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414435108224304896,2461093.6516,12.08,0.05,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 414435108224304896 20260222.1516 12.08CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:54.07 +49:11:17.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.04 00:36:36.73 +46:12:55.9
120.25690 -16.57920 galactic And Second-epoch detections are separated by 7.7" 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 varaible 389151219870290944 | 00:36:37.68 +46:13:02.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 36 36.73 +46 12 55.9 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 varaible 389151219870290944,2461093.6516,12.04,0.05,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
Gaia DR3 varaible 389151219870290944 20260222.1516 12.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:36.73 +46:12:55.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.04 00:30:15.39 +42:20:16.9
118.75903 -20.36204 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 varaible 381942787275748608 | 00:30:14.67 +42:20:12.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 30 15.39 +42 20 16.9 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 varaible 381942787275748608,2461093.6516,12.04,0.05,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
Gaia DR3 varaible 381942787275748608 20260222.1516 12.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:15.39 +42:20:16.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.82 00:37:58.47 +42:40:08.9
120.29658 -20.13371 galactic And Second-epoch detections are separated by 3.2" 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 | ATO J009.4847+42.6626 | 00:37:57.72 +42:40:07.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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 22.1516* 00 37 58.47 +42 40 08.9 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 J009.4847+42.6626,2461093.6516,11.82,0.05,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
ATO J009.4847+42.6626 20260222.1516 11.82CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:58.47 +42:40:08.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.09 00:49:53.72 +41:14:09.2
122.61993 -21.63493 galactic And Second-epoch detections are separated by 5.2" 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 varaible 375047887296724992 | 00:49:53.65 +41:14:18.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 49 53.72 +41 14 09.2 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 varaible 375047887296724992,2461093.6516,12.09,0.05,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 varaible 375047887296724992 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:49:53.72 +41:14:09.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.99 00:41:37.03 +41:40:20.0
120.96559 -21.16203 galactic And Second-epoch detections are separated by 1.9" 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 varaible 381337196893977984 | 00:41:36.69 +41:40:14.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 41 37.03 +41 40 20.0 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 varaible 381337196893977984,2461093.6516,11.99,0.05,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 varaible 381337196893977984 20260222.1516 11.99CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:37.03 +41:40:20.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.81 00:34:52.33 +43:04:54.3
119.72043 -19.68668 galactic And Second-epoch detections are separated by 5.6" 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 varaible 381670241534963712 | 00:34:51.77 +43:04:50.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 34 52.33 +43 04 54.3 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 varaible 381670241534963712,2461093.6516,11.81,0.05,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 varaible 381670241534963712 20260222.1516 11.81CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:52.33 +43:04:54.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.92 00:37:19.26 +45:51:17.0
120.36306 -16.94660 galactic And Second-epoch detections are separated by 3.3" 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 | ATO J009.3361+45.8516 | 00:37:18.47 +45:51:15.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5: 1952IzKry...9...82G BD+45 155
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 37 19.26 +45 51 17.0 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 J009.3361+45.8516,2461093.6516,11.92,0.05,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
ATO J009.3361+45.8516 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:19.26 +45:51:17.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.89 00:27:43.16 +48:12:16.1
118.85416 -14.47939 galactic Cas Second-epoch detections are separated by 5.1" 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 391055608368519936 | 00:27:42.35 +48:12:16.1 (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 22.1516* 00 27 43.16 +48 12 16.1 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391055608368519936,2461093.6516,11.89,0.05,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 391055608368519936 20260222.1516 11.89CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:43.16 +48:12:16.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 36 55.07 +42 20 24.3 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
V0726 And,2461093.6516,11.93,0.05,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
V0726 And 20260222.1516 11.93CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:55.07 +42:20:24.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.80 00:32:07.96 +43:10:49.6
119.19900 -19.55133 galactic And Second-epoch detections are separated by 2.3" 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 varaible 382415680355295744 | 00:32:07.23 +43:10:42.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 32 07.96 +43 10 49.6 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 varaible 382415680355295744,2461093.6516,11.80,0.05,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 varaible 382415680355295744 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:07.96 +43:10:49.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.87 00:30:09.99 +42:25:39.4
118.74977 -20.27134 galactic And Second-epoch detections are separated by 4.7" 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 varaible 382319507447216384 | 00:30:09.22 +42:25:35.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 30 09.99 +42 25 39.4 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 varaible 382319507447216384,2461093.6516,11.87,0.05,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
Gaia DR3 varaible 382319507447216384 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:09.99 +42:25:39.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.95 00:36:22.72 +44:29:44.7
120.10441 -18.29331 galactic And Second-epoch detections are separated by 2.8" 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 varaible 387835860363760384 | 00:36:21.85 +44:29:44.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 36 22.72 +44 29 44.7 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
Gaia DR3 varaible 387835860363760384,2461093.6516,11.95,0.05,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 varaible 387835860363760384 20260222.1516 11.95CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:22.72 +44:29:44.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.84 00:40:12.14 +46:51:11.0
120.93422 -15.97511 galactic Cas Second-epoch detections are separated by 1.7" 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 389958433203149824 | 00:40:11.49 +46:51:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F4 (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 22.1516* 00 40 12.14 +46 51 11.0 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389958433203149824,2461093.6516,11.84,0.05,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 389958433203149824 20260222.1516 11.84CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:12.14 +46:51:11.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.79 00:33:48.89 +43:21:36.8
119.53733 -19.39534 galactic And Second-epoch detections are separated by 5.9" 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 varaible 382432447908248192 | 00:33:49.68 +43:21:43.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 33 48.89 +43 21 36.8 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 varaible 382432447908248192,2461093.6516,11.79,0.05,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 varaible 382432447908248192 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:48.89 +43:21:36.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.80 00:35:41.22 +45:20:46.4
120.03214 -17.43682 galactic And Second-epoch detections are separated by 4.7" 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 varaible 389009279789496576 | 00:35:41.89 +45:20:50.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 35 41.22 +45 20 46.4 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 varaible 389009279789496576,2461093.6516,11.80,0.05,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 varaible 389009279789496576 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:41.22 +45:20:46.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.70 00:31:56.09 +42:33:26.3
119.10756 -20.16957 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 varaible 382300502216005760 | 00:31:54.99 +42:33:25.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 31 56.09 +42 33 26.3 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 varaible 382300502216005760,2461093.6516,11.70,0.05,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 varaible 382300502216005760 20260222.1516 11.70CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:56.09 +42:33:26.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.55 00:31:35.16 +41:47:32.7
118.97219 -20.92665 galactic And Second-epoch detections are separated by 4.4" 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 | Gaia DR3 varaible 381875712769950592 | 00:31:34.42 +41:47:27.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 31 35.16 +41 47 32.7 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 varaible 381875712769950592,2461093.6516,11.55,0.05,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 varaible 381875712769950592 20260222.1516 11.55CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:35.16 +41:47:32.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.70 00:38:58.18 +43:00:35.8
120.50982 -19.80316 galactic And Second-epoch detections are separated by 1.6" 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 | Gaia DR3 varaible 387605684475877760 | 00:38:57.57 +43:00:32.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 38 58.18 +43 00 35.8 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 varaible 387605684475877760,2461093.6516,11.70,0.05,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 varaible 387605684475877760 20260222.1516 11.70CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:58.18 +43:00:35.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.70 00:40:24.37 +44:01:18.8
120.83727 -18.80499 galactic And Second-epoch detections are separated by 7.7" 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 varaible 387773596221245696 | 00:40:25.30 +44:01:28.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 40 24.37 +44 01 18.8 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 varaible 387773596221245696,2461093.6516,11.70,0.05,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 varaible 387773596221245696 20260222.1516 11.70CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:24.37 +44:01:18.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.68 00:35:10.32 +45:16:12.0
119.93221 -17.50699 galactic And Second-epoch detections are separated by 2.2" 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 varaible 389005534578639360 | 00:35:09.14 +45:16:09.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: F8 1952IzKry...9...82G BD+44 121
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 35 10.32 +45 16 12.0 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 varaible 389005534578639360,2461093.6516,11.68,0.05,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 varaible 389005534578639360 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:10.32 +45:16:12.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.57 00:42:01.53 +42:36:59.2
121.08672 -20.22158 galactic And Second-epoch detections are separated by 6.7" 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 varaible 387393925408094336 | 00:42:02.27 +42:37:07.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 42 01.53 +42 36 59.2 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 varaible 387393925408094336,2461093.6516,11.57,0.05,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 varaible 387393925408094336 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:01.53 +42:36:59.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.47 00:48:43.63 +50:52:13.4
122.49470 -11.99906 galactic Cas Second-epoch detections are separated by 3.0" 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 | Gaia DR3 415022453593539328 | 00:48:43.31 +50:52:19.6 (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 22.1516* 00 48 43.63 +50 52 13.4 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415022453593539328,2461093.6516,11.47,0.05,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 415022453593539328 20260222.1516 11.47CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:48:43.63 +50:52:13.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.47 00:29:41.18 +44:27:34.1
118.84798 -18.23973 galactic And Second-epoch detections are separated by 2.8" 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 varaible 388538620092303488 | 00:29:40.21 +44:27:33.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 29 41.18 +44 27 34.1 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 varaible 388538620092303488,2461093.6516,11.47,0.05,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 varaible 388538620092303488 20260222.1516 11.47CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:41.18 +44:27:34.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.40 00:37:32.75 +42:53:15.8
120.22614 -19.91103 galactic And Second-epoch detections are separated by 2.7" 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 | Gaia DR3 varaible 381608673180051200 | 00:37:31.96 +42:53:12.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 37 32.75 +42 53 15.8 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
Gaia DR3 varaible 381608673180051200,2461093.6516,11.40,0.05,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 varaible 381608673180051200 20260222.1516 11.40CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:32.75 +42:53:15.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.49 00:31:45.08 +45:04:33.0
119.28660 -17.65653 galactic And Second-epoch detections are separated by 2.6" 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 J007.9333+45.0864 | 00:31:43.97 +45:04:30.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1952IzKry...9...82G BD+44 105
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 31 45.08 +45 04 33.0 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
ATO J007.9333+45.0864,2461093.6516,11.49,0.05,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 J007.9333+45.0864 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:45.08 +45:04:33.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 31 41.15 +46 40 05.1 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
NSVS 3712255,2461093.6516,11.25,0.05,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
NSVS 3712255 20260222.1516 11.25CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:41.15 +46:40:05.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.38 00:47:50.79 +50:26:10.8
122.34633 -12.43133 galactic Cas Second-epoch detections are separated by 3.7" and 4.8 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 414612267036266496 | 00:47:50.50 +50:26:16.5 (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 22.1516* 00 47 50.79 +50 26 10.8 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414612267036266496,2461093.6516,11.38,0.05,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
Gaia DR3 414612267036266496 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:47:50.79 +50:26:10.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.06 00:37:13.63 +44:16:56.6
120.25043 -18.51536 galactic And Second-epoch detections are separated by 3.3" 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 varaible 387818680493913344 | 00:37:14.57 +44:17:06.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: F8 1952IzKry...9...82G BD+43 117
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 37 13.63 +44 16 56.6 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 varaible 387818680493913344,2461093.6516,11.06,0.05,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 varaible 387818680493913344 20260222.1516 11.06CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:13.63 +44:16:56.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.09 00:32:39.63 +44:55:13.9
119.44206 -17.82395 galactic And Second-epoch detections are separated by 4.2" 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 | ATO J008.1655+44.9085 | 00:32:38.79 +44:55:09.9 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1952IzKry...9...82G BD+44 112
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 32 39.63 +44 55 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
ATO J008.1655+44.9085,2461093.6516,11.09,0.05,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
ATO J008.1655+44.9085 20260222.1516 11.09CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:39.63 +44:55:13.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.10 00:34:08.08 +44:36:16.1
119.69199 -18.15840 galactic And Second-epoch detections are separated by 3.0" 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 varaible 388596786832344192 | 00:34:07.36 +44:36:15.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: A5 1952IzKry...9...82G BD+43 105
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 34 08.08 +44 36 16.1 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 varaible 388596786832344192,2461093.6516,11.10,0.05,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 varaible 388596786832344192 20260222.1516 11.10CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:08.08 +44:36:16.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.06 00:38:38.51 +43:48:31.3
120.49080 -19.00239 galactic And Second-epoch detections are separated by 4.1" 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 | Gaia DR3 varaible 387754565222316416 | 00:38:39.53 +43:48:41.4 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 38 38.51 +43 48 31.3 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 varaible 387754565222316416,2461093.6516,11.06,0.05,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 varaible 387754565222316416 20260222.1516 11.06CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:38.51 +43:48:31.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.96 00:33:43.43 +46:08:52.8
119.73171 -16.61365 galactic And Second-epoch detections are separated by 1.6" 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 varaible 389115588819807744 | 00:33:42.84 +46:08:51.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: F5 1952IzKry...9...82G BD+45 142
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 33 43.43 +46 08 52.8 11.0 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 varaible 389115588819807744,2461093.6516,10.96,0.05,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 varaible 389115588819807744 20260222.1516 10.96CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:43.43 +46:08:52.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.79 00:39:21.80 +43:26:05.0
120.60864 -19.38255 galactic And Second-epoch detections are separated by 3.0" 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 varaible 387641345587578624 | 00:39:22.47 +43:26:12.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 39 21.80 +43 26 05.0 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 varaible 387641345587578624,2461093.6516,10.79,0.05,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 varaible 387641345587578624 20260222.1516 10.79CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:21.80 +43:26:05.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.65 00:31:38.64 +43:08:45.1
119.10178 -19.57863 galactic And Second-epoch detections are separated by 4.8" 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 varaible 382456431004893824 | 00:31:37.80 +43:08:34.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 31 38.64 +43 08 45.1 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 varaible 382456431004893824,2461093.6516,10.65,0.05,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 varaible 382456431004893824 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:38.64 +43:08:45.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.47 00:35:07.66 +44:27:31.7
119.86735 -18.31587 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 | Gaia DR3 varaible 388580294159599104 | 00:35:06.84 +44:27:30.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: F5 1952IzKry...9...82G BD+43 108
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 35 07.66 +44 27 31.7 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 varaible 388580294159599104,2461093.6516,10.47,0.05,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 varaible 388580294159599104 20260222.1516 10.47CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:07.66 +44:27:31.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.46 00:42:44.69 +49:22:32.1
121.47706 -13.47161 galactic Cas Second-epoch detections are separated by 5.2" and 5.0 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 414683426055245312 | 00:42:45.79 +49:22:27.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1952CoRut..32....1H BD+48 213
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 42 44.69 +49 22 32.1 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414683426055245312,2461093.6516,10.46,0.05,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 414683426055245312 20260222.1516 10.46CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:44.69 +49:22:32.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.40 00:29:35.36 +48:43:49.5
119.22206 -13.98389 galactic Cas Second-epoch detections are separated by 4.7" 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 391141610793721088 | 00:29:36.76 +48:43:51.3 (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 22.1516* 00 29 35.36 +48 43 49.5 10.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391141610793721088,2461093.6516,10.40,0.05,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 391141610793721088 20260222.1516 10.40CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:35.36 +48:43:49.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.54 00:41:50.00 +50:22:44.0
121.36399 -12.46362 galactic Cas Second-epoch detections are separated by 3.0" and 5.0 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 414842580363440384 | 00:41:50.82 +50:22:40.9 (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 22.1516* 00 41 50.00 +50 22 44.0 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414842580363440384,2461093.6516,10.54,0.05,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 414842580363440384 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:50.00 +50:22:44.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.53 00:35:37.92 +50:50:42.2
120.38280 -11.94845 galactic Cas Second-epoch detections are separated by 6.3" 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 415582925347690752 | 00:35:39.39 +50:50:39.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1927AnHar.100...33C HD 232224
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 35 37.92 +50 50 42.2 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415582925347690752,2461093.6516,10.53,0.05,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 415582925347690752 20260222.1516 10.53CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:37.92 +50:50:42.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.46 00:28:04.77 +48:42:28.0
118.96437 -13.98394 galactic Cas Second-epoch detections are separated by 2.3" and 5.1 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 J007.0138+48.6997 | 00:28:06.04 +48:42:25.0 (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 22.1516* 00 28 04.77 +48 42 28.0 10.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J007.0138+48.6997,2461093.6516,10.46,0.05,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 J007.0138+48.6997 20260222.1516 10.46CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:04.77 +48:42:28.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.66 00:27:47.01 +48:44:55.4
118.91826 -13.93860 galactic Cas Second-epoch detections are separated by 4.9" 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 391185827479873152 | 00:27:48.26 +48:44:51.2 (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 22.1516* 00 27 47.01 +48 44 55.4 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391185827479873152,2461093.6516,10.66,0.05,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 391185827479873152 20260222.1516 10.66CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:47.01 +48:44:55.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.72 00:39:27.37 +49:30:14.0
120.93341 -13.32136 galactic Cas Second-epoch detections are separated by 5.5" 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 391429236164161664 | 00:39:28.19 +49:30:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1952CoRut..32....1H BD+48 193
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 39 27.37 +49 30 14.0 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391429236164161664,2461093.6516,10.72,0.05,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
Gaia DR3 391429236164161664 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:27.37 +49:30:14.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.78 00:40:07.46 +50:58:10.9
121.11236 -11.86208 galactic Cas Second-epoch detections are separated by 3.7" and 5.0 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 415614162647824000 | 00:40:08.55 +50:58:07.0 (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 22.1516* 00 40 07.46 +50 58 10.9 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415614162647824000,2461093.6516,10.78,0.05,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 415614162647824000 20260222.1516 10.78CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:07.46 +50:58:10.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.79 00:28:10.52 +50:28:13.3
119.14818 -12.23041 galactic Cas Second-epoch detections are separated by 5.8" 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 391763964436082816 | 00:28:11.70 +50:28:06.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1952CoRut..32....1H BD+49 97
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 28 10.52 +50 28 13.3 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391763964436082816,2461093.6516,10.79,0.05,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 391763964436082816 20260222.1516 10.79CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:10.52 +50:28:13.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 40 25.51 +50 06 20.4 10.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414741665811284096,2461093.6516,10.84,0.05,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 414741665811284096 20260222.1516 10.84CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:25.51 +50:06:20.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.77 00:27:37.26 +46:39:48.3
118.68446 -16.01182 galactic And Second-epoch detections are separated by 3.2" 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 389385965601307392 | 00:27:38.41 +46:39:47.2 (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 22.1516* 00 27 37.26 +46 39 48.3 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 389385965601307392,2461093.6516,10.77,0.05,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 389385965601307392 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:37.26 +46:39:48.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 10.95 00:37:13.26 +49:18:30.1
120.54962 -13.49761 galactic Cas Second-epoch detections are separated by 4.2" and 5.0 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 J009.3217+49.3088 | 00:37:14.56 +49:18:31.3 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A5 1952CoRut..32....1H BD+48 184
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 37 13.26 +49 18 30.1 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J009.3217+49.3088,2461093.6516,10.95,0.05,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 J009.3217+49.3088 20260222.1516 10.95CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:37:13.26 +49:18:30.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.03 00:34:29.11 +49:44:40.1
120.12221 -13.03477 galactic Cas Second-epoch detections are separated by 2.2" 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 391482974796699648 | 00:34:30.53 +49:44:38.9 (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 22.1516* 00 34 29.11 +49 44 40.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391482974796699648,2461093.6516,11.03,0.05,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 391482974796699648 20260222.1516 11.03CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:29.11 +49:44:40.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.01 00:40:02.38 +48:45:55.9
120.99604 -14.06337 galactic Cas Second-epoch detections are separated by 5.5" and 4.1 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 390541857261634304 | 00:40:03.18 +48:45:53.6 (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 22.1516* 00 40 02.38 +48 45 55.9 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390541857261634304,2461093.6516,11.01,0.05,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 390541857261634304 20260222.1516 11.01CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:02.38 +48:45:55.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.04 00:29:10.89 +50:35:55.5
119.32293 -12.11697 galactic Cas Second-epoch detections are separated by 5.9" 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 | ATO J007.2887+50.5922 | 00:29:11.92 +50:35:50.6 (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 22.1516* 00 29 10.89 +50 35 55.5 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J007.2887+50.5922,2461093.6516,11.04,0.05,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
ATO J007.2887+50.5922 20260222.1516 11.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:10.89 +50:35:55.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.16 00:40:22.63 +48:24:40.9
121.03713 -14.41969 galactic Cas Second-epoch detections are separated by 4.0" and 4.7 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 390529526414760832 | 00:40:23.65 +48:24:38.8 (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 22.1516* 00 40 22.63 +48 24 40.9 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390529526414760832,2461093.6516,11.16,0.05,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 390529526414760832 20260222.1516 11.16CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:22.63 +48:24:40.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.19 00:40:47.98 +50:22:54.8
121.19549 -12.45399 galactic Cas Second-epoch detections are separated by 1.3" 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 414752592208164352 | 00:40:49.01 +50:22:48.8 (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 22.1516* 00 40 47.98 +50 22 54.8 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414752592208164352,2461093.6516,11.19,0.05,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 414752592208164352 20260222.1516 11.19CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:47.98 +50:22:54.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.11 00:39:44.84 +48:49:09.3
120.94903 -14.00748 galactic Cas Second-epoch detections are separated by 7.2" and 3.6 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 390545194455385984 | 00:39:45.69 +48:49:08.3 (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 22.1516* 00 39 44.84 +48 49 09.3 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390545194455385984,2461093.6516,11.11,0.05,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 390545194455385984 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:44.84 +48:49:09.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 30 43.02 +50 40 39.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391739848198259712,2461093.6516,11.16,0.05,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 391739848198259712 20260222.1516 11.16CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:43.02 +50:40:39.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.28 00:41:56.98 +50:23:36.6
121.38354 -12.44972 galactic Cas Second-epoch detections are separated by 3.5" and 5.1 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 414842271127410304 | 00:41:57.90 +50:23:45.0 (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 22.1516* 00 41 56.98 +50 23 36.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414842271127410304,2461093.6516,11.28,0.05,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 414842271127410304 20260222.1516 11.28CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:41:56.98 +50:23:36.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.23 00:27:32.70 +47:03:25.6
118.71035 -15.61870 galactic Cas Second-epoch detections are separated by 4.8" 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 | Gaia DR3 389492377711630592 | 00:27:33.83 +47:03:24.5 (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 22.1516* 00 27 32.70 +47 03 25.6 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389492377711630592,2461093.6516,11.23,0.05,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 389492377711630592 20260222.1516 11.23CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:32.70 +47:03:25.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.30 00:31:52.49 +46:21:57.7
119.41648 -16.37214 galactic And Second-epoch detections are separated by 4.5" 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 varaible 389133765121198336 | 00:31:53.87 +46:22:02.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: G0: 1952IzKry...9...82G BD+45 125
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 31 52.49 +46 21 57.7 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 varaible 389133765121198336,2461093.6516,11.30,0.05,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 varaible 389133765121198336 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:52.49 +46:21:57.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.31 00:28:25.81 +46:51:48.6
118.84755 -15.82571 galactic Cas Second-epoch detections are separated by 8.3" and 4.1 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 389349338122418816 | 00:28:26.88 +46:51:51.5 (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 22.1516* 00 28 25.81 +46 51 48.6 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389349338122418816,2461093.6516,11.31,0.05,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
Gaia DR3 389349338122418816 20260222.1516 11.31CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:25.81 +46:51:48.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.40 00:33:42.49 +47:24:29.0
119.82267 -15.35663 galactic Cas Second-epoch detections are separated by 3.3" and 5.0 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 J008.4220+47.4126 | 00:33:43.62 +47:24:31.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F1: 1952IzKry...9...82G BD+46 109
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 33 42.49 +47 24 29.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J008.4220+47.4126,2461093.6516,11.40,0.05,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
ATO J008.4220+47.4126 20260222.1516 11.40CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:42.49 +47:24:29.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.48 00:34:42.15 +50:28:57.4
120.20852 -12.30062 galactic Cas Second-epoch detections are separated by 7.1" 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 415550150454731776 | 00:34:43.03 +50:28:49.7 (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 22.1516* 00 34 42.15 +50 28 57.4 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415550150454731776,2461093.6516,11.48,0.05,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 415550150454731776 20260222.1516 11.48CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:42.15 +50:28:57.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.39 00:27:48.06 +50:07:21.0
119.05408 -12.57119 galactic Cas Second-epoch detections are separated by 6.4" 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 391658621779517056 | 00:27:49.10 +50:07:16.6 (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 22.1516* 00 27 48.06 +50 07 21.0 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391658621779517056,2461093.6516,11.39,0.05,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
Gaia DR3 391658621779517056 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:48.06 +50:07:21.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.48 00:36:47.71 +50:42:53.9
120.56241 -12.08940 galactic Cas Second-epoch detections are separated by 5.7" 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 415566814930124160 | 00:36:49.52 +50:42:56.9 (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 22.1516* 00 36 47.71 +50 42 53.9 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415566814930124160,2461093.6516,11.48,0.05,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 415566814930124160 20260222.1516 11.48CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:47.71 +50:42:53.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 31 47.45 +47 44 57.0 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390980424964297984,2461093.6516,11.46,0.05,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 390980424964297984 20260222.1516 11.46CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:47.45 +47:44:57.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.49 00:27:51.93 +46:50:39.7
118.74579 -15.83570 galactic Cas Second-epoch detections are separated by 3.9" 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 | ATO J006.9732+46.8525 | 00:27:53.43 +46:50:43.7 (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 22.1516* 00 27 51.93 +46 50 39.7 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.9732+46.8525,2461093.6516,11.49,0.05,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 J006.9732+46.8525 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:51.93 +46:50:39.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.46 00:33:00.95 +44:43:33.1
119.49258 -18.02283 galactic And Second-epoch detections are separated by 4.9" 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 varaible 388602116890169088 | 00:33:01.74 +44:43:47.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: K0 1984AJ.....89..702L BD+43 100
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 33 00.95 +44 43 33.1 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 varaible 388602116890169088,2461093.6516,11.46,0.05,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 varaible 388602116890169088 20260222.1516 11.46CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:00.95 +44:43:33.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 25 56.30 +50 25 36.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394676643756300160,2461093.6516,11.46,0.05,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 394676643756300160 20260222.1516 11.46CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:25:56.30 +50:25:36.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.55 00:32:36.67 +50:35:50.6
119.87766 -12.16268 galactic Cas Second-epoch detections are separated by 5.7" 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 391724729916201728 | 00:32:38.16 +50:35:42.5 (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 22.1516* 00 32 36.67 +50 35 50.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391724729916201728,2461093.6516,11.55,0.05,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 391724729916201728 20260222.1516 11.55CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:36.67 +50:35:50.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.53 00:32:52.46 +47:20:32.6
119.67168 -15.41181 galactic Cas Second-epoch detections are separated by 4.3" 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 390778256562008320 | 00:32:53.76 +47:20:33.3 (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 22.1516* 00 32 52.46 +47 20 32.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390778256562008320,2461093.6516,11.53,0.05,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 390778256562008320 20260222.1516 11.53CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:52.46 +47:20:32.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.56 00:36:54.48 +41:38:02.8
120.02149 -21.15551 galactic And Second-epoch detections are separated by 4.3" 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 varaible 381428933091943040 | 00:36:54.79 +41:38:20.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 36 54.48 +41 38 02.8 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 varaible 381428933091943040,2461093.6516,11.56,0.05,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 varaible 381428933091943040 20260222.1516 11.56CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:54.48 +41:38:02.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.56 00:34:00.37 +47:26:14.4
119.87696 -15.33099 galactic Cas Second-epoch detections are separated by 2.4" 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 390770766138089472 | 00:34:01.93 +47:26:17.8 (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 22.1516* 00 34 00.37 +47 26 14.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390770766138089472,2461093.6516,11.56,0.05,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 390770766138089472 20260222.1516 11.56CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:00.37 +47:26:14.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.56 00:33:23.87 +47:46:20.3
119.79573 -14.98956 galactic Cas Second-epoch detections are separated by 4.6" and 5.1 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 390819247728739072 | 00:33:25.40 +47:46:25.8 (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 22.1516* 00 33 23.87 +47 46 20.3 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390819247728739072,2461093.6516,11.56,0.05,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 390819247728739072 20260222.1516 11.56CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:23.87 +47:46:20.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.57 00:34:15.21 +45:44:27.2
119.79759 -17.02625 galactic And Second-epoch detections are separated by 6.8" 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 varaible 389056146472730368 | 00:34:16.03 +45:44:34.5 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 34 15.21 +45 44 27.2 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 varaible 389056146472730368,2461093.6516,11.57,0.05,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 varaible 389056146472730368 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:15.21 +45:44:27.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.55 00:27:06.72 +48:44:44.8
118.80444 -13.93092 galactic Cas Second-epoch detections are separated by 3.7" and 5.3 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 391104227398100736 | 00:27:07.82 +48:44:40.5 (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 22.1516* 00 27 06.72 +48 44 44.8 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391104227398100736,2461093.6516,11.55,0.05,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 391104227398100736 20260222.1516 11.55CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:06.72 +48:44:44.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.61 00:30:11.27 +47:42:51.6
119.23407 -15.00478 galactic Cas Second-epoch detections are separated by 1.8" and 5.0 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 390989087917542784 | 00:30:12.73 +47:42:52.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A5 1952IzKry...9...82G BD+46 93
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 30 11.27 +47 42 51.6 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390989087917542784,2461093.6516,11.61,0.05,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 390989087917542784 20260222.1516 11.61CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:11.27 +47:42:51.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.57 00:33:30.94 +50:15:17.7
119.99915 -12.51475 galactic Cas Second-epoch detections are separated by 6.2" and 4.5 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 391710264466428032 | 00:33:31.65 +50:15:16.6 (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 22.1516* 00 33 30.94 +50 15 17.7 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391710264466428032,2461093.6516,11.57,0.05,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 391710264466428032 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:30.94 +50:15:17.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.66 00:27:22.09 +50:06:14.5
118.98151 -12.58301 galactic Cas Second-epoch detections are separated by 4.6" 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 391660163667451392 | 00:27:23.30 +50:06:10.0 (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 22.1516* 00 27 22.09 +50 06 14.5 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391660163667451392,2461093.6516,11.66,0.05,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 391660163667451392 20260222.1516 11.66CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:22.09 +50:06:14.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.79 00:34:06.84 +50:18:15.7
120.10037 -12.47212 galactic Cas Second-epoch detections are separated by 2.5" 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 391528948124124544 | 00:34:08.26 +50:18:11.1 (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 22.1516* 00 34 06.84 +50 18 15.7 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391528948124124544,2461093.6516,11.79,0.05,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 391528948124124544 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:06.84 +50:18:15.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.69 00:29:57.12 +50:51:20.4
119.46989 -11.87160 galactic Cas Second-epoch detections are separated by 6.0" 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 391791868842034304 | 00:29:58.08 +50:51:15.4 (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 22.1516* 00 29 57.12 +50 51 20.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391791868842034304,2461093.6516,11.69,0.05,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 391791868842034304 20260222.1516 11.69CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:57.12 +50:51:20.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.71 00:26:39.99 +50:38:49.0
118.92138 -12.03181 galactic Cas Second-epoch detections are separated by 2.5" and 4.1 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 J006.6731+50.6581 | 00:26:41.32 +50:38:51.4 (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 22.1516* 00 26 39.99 +50 38 49.0 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.6731+50.6581,2461093.6516,11.71,0.05,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 J006.6731+50.6581 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:39.99 +50:38:49.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.71 00:28:26.73 +47:32:06.4
118.91473 -15.15722 galactic Cas Second-epoch detections are separated by 8.1" 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 | Gaia DR3 389529073912374656 | 00:28:28.25 +47:32:13.9 (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 22.1516* 00 28 26.73 +47 32 06.4 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389529073912374656,2461093.6516,11.71,0.05,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 389529073912374656 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:26.73 +47:32:06.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.74 00:32:50.24 +48:02:08.2
119.71884 -14.72006 galactic Cas Second-epoch detections are separated by 4.5" and 4.5 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 390826531993211648 | 00:32:51.39 +48:02:10.5 (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 22.1516* 00 32 50.24 +48 02 08.2 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390826531993211648,2461093.6516,11.74,0.05,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 390826531993211648 20260222.1516 11.74CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:50.24 +48:02:08.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.82 00:32:55.26 +50:52:16.6
119.94839 -11.89317 galactic Cas Second-epoch detections are separated by 6.2" 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 | ATO J008.2201+50.8658 | 00:32:55.96 +50:52:11.4 (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 22.1516* 00 32 55.26 +50 52 16.6 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J008.2201+50.8658,2461093.6516,11.82,0.05,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
ATO J008.2201+50.8658 20260222.1516 11.82CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:55.26 +50:52:16.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.74 00:33:11.55 +46:20:28.4
119.65081 -16.41426 galactic And Second-epoch detections are separated by 4.5" and 4.5 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 varaible 389211555569897216 | 00:33:13.05 +46:20:25.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 33 11.55 +46 20 28.4 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 varaible 389211555569897216,2461093.6516,11.74,0.05,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 varaible 389211555569897216 20260222.1516 11.74CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:11.55 +46:20:28.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.76 00:26:08.30 +50:36:53.2
118.83290 -12.05551 galactic Cas Second-epoch detections are separated by 6.6" 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 394773332057503488 | 00:26:09.29 +50:36:52.8 (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 22.1516* 00 26 08.30 +50 36 53.2 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394773332057503488,2461093.6516,11.76,0.05,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 394773332057503488 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:08.30 +50:36:53.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.84 00:31:26.81 +49:04:41.2
119.56523 -13.66291 galactic Cas Second-epoch detections are separated by 1.7" and 4.0 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 391161951761028480 | 00:31:29.92 +49:04:16.0 (Gaia DR3) | DSCT/GDOR (local) | (local) | Gaia3var=NOT_AVAILABLE SpType: A2 1952CoRut..32....1H BD+48 153
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 31 26.81 +49 04 41.2 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391161951761028480,2461093.6516,11.84,0.05,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 391161951761028480 20260222.1516 11.84CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:26.81 +49:04:41.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.86 00:32:11.73 +50:25:33.3
119.79698 -12.32867 galactic Cas Second-epoch detections are separated by 1.6" and 5.0 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 J008.0437+50.4210 | 00:32:12.53 +50:25:27.9 (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 22.1516* 00 32 11.73 +50 25 33.3 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J008.0437+50.4210,2461093.6516,11.86,0.05,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 J008.0437+50.4210 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:11.73 +50:25:33.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.86 00:40:02.87 +49:44:40.7
121.04324 -13.08534 galactic Cas Second-epoch detections are separated by 8.7" and 4.6 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 414706618878191744 | 00:40:03.50 +49:44:36.3 (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 22.1516* 00 40 02.87 +49 44 40.7 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414706618878191744,2461093.6516,11.86,0.05,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
Gaia DR3 414706618878191744 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:02.87 +49:44:40.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.80 00:27:11.90 +50:08:47.8
118.95794 -12.53801 galactic Cas Second-epoch detections are separated by 5.8" 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 391661130034023296 | 00:27:13.41 +50:08:42.4 (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 22.1516* 00 27 11.90 +50 08 47.8 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391661130034023296,2461093.6516,11.80,0.05,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 391661130034023296 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:11.90 +50:08:47.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.82 00:31:49.76 +49:28:28.9
119.66138 -13.27249 galactic Cas Second-epoch detections are separated by 8.2" 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 391572378834213376 | 00:31:51.00 +49:28:30.7 (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 22.1516* 00 31 49.76 +49 28 28.9 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391572378834213376,2461093.6516,11.82,0.05,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 391572378834213376 20260222.1516 11.82CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:49.76 +49:28:28.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.87 00:31:45.63 +45:04:58.0
119.28888 -17.64974 galactic And Second-epoch detections are separated by 2.5" 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 | ATO J007.9333+45.0864 | 00:31:43.97 +45:04:30.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: A2 1952IzKry...9...82G BD+44 105
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 31 45.63 +45 04 58.0 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 J007.9333+45.0864,2461093.6516,11.87,0.05,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 J007.9333+45.0864 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:45.63 +45:04:58.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.89 00:42:16.59 +50:56:56.4
121.45752 -11.89652 galactic Cas Second-epoch detections are separated by 4.6" and 5.0 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 | Large-amplitude variable Gaia DR2 414886487810193920 | 00:42:18.20 +50:56:55.7 (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 22.1516* 00 42 16.59 +50 56 56.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 414886487810193920,2461093.6516,11.89,0.05,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
Large-amplitude variable Gaia DR2 414886487810193920 20260222.1516 11.89CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:16.59 +50:56:56.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.89 00:26:00.85 +49:45:49.8
118.72491 -12.90013 galactic Cas Second-epoch detections are separated by 6.3" 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 | ATO J006.4940+49.7621 | 00:26:01.47 +49:45:46.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: K0 1958PMcCO..13b....V AG+49 62
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 26 00.85 +49 45 49.8 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.4940+49.7621,2461093.6516,11.89,0.05,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 J006.4940+49.7621 20260222.1516 11.89CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:00.85 +49:45:49.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.91 00:36:15.62 +50:44:15.3
120.47738 -12.06182 galactic Cas Second-epoch detections are separated by 1.3" and 4.7 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 415570319621031936 | 00:36:16.57 +50:44:11.9 (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 22.1516* 00 36 15.62 +50 44 15.3 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415570319621031936,2461093.6516,11.91,0.05,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 415570319621031936 20260222.1516 11.91CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:15.62 +50:44:15.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.99 00:46:23.83 +50:54:06.0
122.11957 -11.96213 galactic Cas Second-epoch detections are separated by 6.3" and 4.1 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 J011.6127+50.8980 | 00:46:24.54 +50:54:03.4 (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 22.1516* 00 46 23.83 +50 54 06.0 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J011.6127+50.8980,2461093.6516,11.99,0.05,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 J011.6127+50.8980 20260222.1516 11.99CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:23.83 +50:54:06.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.95 00:40:56.78 +48:54:08.4
121.15584 -13.93323 galactic Cas Second-epoch detections are separated by 8.1" 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 390625660663901568 | 00:40:57.83 +48:54:05.6 (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 22.1516* 00 40 56.78 +48 54 08.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390625660663901568,2461093.6516,11.95,0.05,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 390625660663901568 20260222.1516 11.95CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:56.78 +48:54:08.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.94 00:33:15.77 +49:37:33.7
119.91122 -13.13909 galactic Cas Second-epoch detections are separated by 6.1" and 5.0 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 | Large-amplitude variable Gaia DR2 391390340939844736 | 00:33:18.20 +49:37:37.4 (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 22.1516* 00 33 15.77 +49 37 33.7 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 391390340939844736,2461093.6516,11.94,0.05,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
Large-amplitude variable Gaia DR2 391390340939844736 20260222.1516 11.94CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:15.77 +49:37:33.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.93 00:32:21.55 +48:47:50.3
119.69648 -13.95455 galactic Cas Second-epoch detections are separated by 6.2" and 4.5 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 391153907281211776 | 00:32:22.31 +48:47:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.364+/-0.122 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 32 21.55 +48 47 50.3 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391153907281211776,2461093.6516,11.93,0.05,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 391153907281211776 20260222.1516 11.93CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:21.55 +48:47:50.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.95 00:26:52.85 +50:27:01.0
118.93637 -12.23086 galactic Cas Second-epoch detections are separated by 6.9" 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 394674547812264448 | 00:26:54.34 +50:26:55.3 (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 22.1516* 00 26 52.85 +50 27 01.0 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394674547812264448,2461093.6516,11.95,0.05,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 394674547812264448 20260222.1516 11.95CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:52.85 +50:27:01.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.85 00:34:21.95 +48:11:20.7
119.99322 -14.58523 galactic Cas Second-epoch detections are separated by 7.3" and 3.3 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 390914080603432576 | 00:34:22.67 +48:11:22.7 (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 22.1516* 00 34 21.95 +48 11 20.7 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390914080603432576,2461093.6516,11.85,0.05,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
Gaia DR3 390914080603432576 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:21.95 +48:11:20.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.95 00:32:46.50 +50:19:34.2
119.88361 -12.43509 galactic Cas Second-epoch detections are separated by 2.4" and 5.0 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 391714318913105152 | 00:32:48.33 +50:19:31.9 (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 22.1516* 00 32 46.50 +50 19 34.2 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391714318913105152,2461093.6516,11.95,0.05,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 391714318913105152 20260222.1516 11.95CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:46.50 +50:19:34.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.99 00:32:11.08 +50:39:26.7
119.81331 -12.09771 galactic Cas Second-epoch detections are separated by 5.2" 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 391736824541621760 | 00:32:12.14 +50:39:23.1 (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 22.1516* 00 32 11.08 +50 39 26.7 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391736824541621760,2461093.6516,11.99,0.05,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 391736824541621760 20260222.1516 11.99CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:11.08 +50:39:26.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.99 00:28:11.47 +50:09:06.6
119.12065 -12.54781 galactic Cas Second-epoch detections are separated by 4.4" 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 391664737812358784 | 00:28:12.15 +50:09:03.4 (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 22.1516* 00 28 11.47 +50 09 06.6 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391664737812358784,2461093.6516,11.99,0.05,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 391664737812358784 20260222.1516 11.99CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:11.47 +50:09:06.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.04 00:27:46.97 +47:26:24.2
118.79001 -15.24137 galactic Cas Second-epoch detections are separated by 5.5" 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 | Gaia DR3 389527562085754496 | 00:27:48.52 +47:26:29.7 (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 22.1516* 00 27 46.97 +47 26 24.2 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389527562085754496,2461093.6516,12.04,0.05,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
Gaia DR3 389527562085754496 20260222.1516 12.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:46.97 +47:26:24.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.99 00:31:34.11 +50:08:03.2
119.67149 -12.61170 galactic Cas Second-epoch detections are separated by 4.8" 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 391694046667272064 | 00:31:34.29 +50:07:57.4 (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 22.1516* 00 31 34.11 +50 08 03.2 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391694046667272064,2461093.6516,11.99,0.05,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 391694046667272064 20260222.1516 11.99CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:34.11 +50:08:03.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 30 19.59 +41 10 31.5 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
V0491 And,2461093.6516,11.98,0.05,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
V0491 And 20260222.1516 11.98CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:19.59 +41:10:31.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.06 00:29:39.45 +50:03:41.8
119.35234 -12.65870 galactic Cas Second-epoch detections are separated by 4.5" and 5.0 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 391649413369136384 | 00:29:40.63 +50:03:49.8 (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 22.1516* 00 29 39.45 +50 03 41.8 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391649413369136384,2461093.6516,12.06,0.05,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 391649413369136384 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:39.45 +50:03:41.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 31 05.24 +50 41 52.8 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391740054357014656,2461093.6516,12.06,0.05,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 391740054357014656 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:05.24 +50:41:52.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.15 00:44:15.48 +50:16:51.3
121.75680 -12.57445 galactic Cas Second-epoch detections are separated by 4.1" and 4.6 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 414785405759124480 | 00:44:16.49 +50:16:53.5 (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 22.1516* 00 44 15.48 +50 16 51.3 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414785405759124480,2461093.6516,12.15,0.05,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 414785405759124480 20260222.1516 12.15CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:15.48 +50:16:51.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.12 00:44:01.83 +50:08:46.5
121.71551 -12.70800 galactic Cas Second-epoch detections are separated by 7.9" and 4.2 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 414777228141131904 | 00:44:02.70 +50:08:43.4 (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 22.1516* 00 44 01.83 +50 08 46.5 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414777228141131904,2461093.6516,12.12,0.05,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 414777228141131904 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:44:01.83 +50:08:46.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.19 00:47:43.48 +49:58:08.9
122.31939 -12.89819 galactic Cas Second-epoch detections are separated by 6.8" and 4.2 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 414575845710452864 | 00:47:44.45 +49:58:05.9 (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 22.1516* 00 47 43.48 +49 58 08.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414575845710452864,2461093.6516,12.19,0.05,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 414575845710452864 20260222.1516 12.19CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:47:43.48 +49:58:08.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.11 00:29:39.05 +50:11:50.6
119.36329 -12.52334 galactic Cas Second-epoch detections are separated by 5.2" 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 391744314964462464 | 00:29:40.36 +50:11:46.6 (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 22.1516* 00 29 39.05 +50 11 50.6 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391744314964462464,2461093.6516,12.11,0.05,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 391744314964462464 20260222.1516 12.11CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:39.05 +50:11:50.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.16 00:34:30.33 +50:35:31.2
120.18404 -12.18939 galactic Cas Second-epoch detections are separated by 5.1" 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 415552555638723968 | 00:34:31.58 +50:35:29.6 (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 22.1516* 00 34 30.33 +50 35 31.2 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415552555638723968,2461093.6516,12.16,0.05,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 415552555638723968 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:30.33 +50:35:31.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 38 29.50 +49 12 54.5 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391398514258621568,2461093.6516,12.26,0.05,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 391398514258621568 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:29.50 +49:12:54.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 29 53.31 +48 07 15.7 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391025096921154816,2461093.6516,12.14,0.05,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 391025096921154816 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:53.31 +48:07:15.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.10 00:28:47.26 +48:40:22.0
119.08100 -14.02954 galactic Cas Second-epoch detections are separated by 6.0" and 4.6 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 391181635590033920 | 00:28:48.28 +48:40:22.5 (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 22.1516* 00 28 47.26 +48 40 22.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391181635590033920,2461093.6516,12.10,0.05,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 391181635590033920 20260222.1516 12.10CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:47.26 +48:40:22.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 31 06.74 +48 27 58.3 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J003107.99+482813.2,2461093.6516,12.18,0.05,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
ZTF J003107.99+482813.2 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:06.74 +48:27:58.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.20 00:31:34.55 +50:52:17.7
119.73217 -11.87672 galactic Cas Second-epoch detections are separated by 7.5" 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 | Gaia DR3 415761291049708928 | 00:31:35.09 +50:52:13.7 (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 22.1516* 00 31 34.55 +50 52 17.7 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415761291049708928,2461093.6516,12.20,0.05,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
Gaia DR3 415761291049708928 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:34.55 +50:52:17.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.05 00:39:40.82 +49:10:20.1
120.95476 -13.65436 galactic Cas Second-epoch detections are separated by 4.3" and 4.2 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 390649751135402752 | 00:39:41.81 +49:10:18.1 (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 22.1516* 00 39 40.82 +49 10 20.1 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390649751135402752,2461093.6516,12.05,0.05,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 390649751135402752 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:40.82 +49:10:20.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.16 00:31:10.55 +50:45:01.0
119.65793 -11.99262 galactic Cas Second-epoch detections are separated by 4.6" 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 391741085149158400 | 00:31:11.72 +50:44:55.4 (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 22.1516* 00 31 10.55 +50 45 01.0 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391741085149158400,2461093.6516,12.16,0.05,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 391741085149158400 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:10.55 +50:45:01.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.15 00:25:16.94 +50:35:20.6
118.69205 -12.06725 galactic Cas Second-epoch detections are separated by 7.0" 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 | Large-amplitude variable Gaia DR2 394690456371077760 | 00:25:18.44 +50:35:14.8 (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 22.1516* 00 25 16.94 +50 35 20.6 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 394690456371077760,2461093.6516,12.15,0.05,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
Large-amplitude variable Gaia DR2 394690456371077760 20260222.1516 12.15CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:25:16.94 +50:35:20.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.21 00:28:10.60 +50:15:18.0
119.12805 -12.44487 galactic Cas Second-epoch detections are separated by 5.8" 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 391666936836183936 | 00:28:12.01 +50:15:11.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: B 1965ZA.....62....6B BD+49 96
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 28 10.60 +50 15 18.0 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391666936836183936,2461093.6516,12.21,0.05,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 391666936836183936 20260222.1516 12.21CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:10.60 +50:15:18.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.16 00:29:11.46 +47:45:53.1
119.06580 -14.93993 galactic Cas Second-epoch detections are separated by 5.2" and 4.6 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 390991699257539200 | 00:29:12.27 +47:45:54.8 (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 22.1516* 00 29 11.46 +47 45 53.1 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390991699257539200,2461093.6516,12.16,0.05,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 390991699257539200 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:11.46 +47:45:53.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.16 00:33:16.34 +50:44:11.8
119.99496 -12.03152 galactic Cas Second-epoch detections are separated by 2.7" and 5.1 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 415745691726459264 | 00:33:17.05 +50:44:09.9 (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 22.1516* 00 33 16.34 +50 44 11.8 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415745691726459264,2461093.6516,12.16,0.05,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 415745691726459264 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:16.34 +50:44:11.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 49 44.43 +41 02 37.4 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 375009297014343808,2461093.6516,12.38,0.05,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 375009297014343808 20260222.1516 12.38CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:49:44.43 +41:02:37.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.21 00:30:07.34 +50:12:32.0
119.44130 -12.51834 galactic Cas Second-epoch detections are separated by 5.4" 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 391743799568389120 | 00:30:08.24 +50:12:34.6 (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 22.1516* 00 30 07.34 +50 12 32.0 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391743799568389120,2461093.6516,12.21,0.05,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 391743799568389120 20260222.1516 12.21CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:07.34 +50:12:32.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.26 00:30:08.25 +49:12:19.3
119.35645 -13.51846 galactic Cas Second-epoch detections are separated by 7.7" and 5.0 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 391178547514649856 | 00:30:09.58 +49:12:21.9 (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 22.1516* 00 30 08.25 +49 12 19.3 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391178547514649856,2461093.6516,12.26,0.05,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 391178547514649856 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:08.25 +49:12:19.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.23 00:29:53.44 +50:11:02.4
119.40128 -12.53998 galactic Cas Second-epoch detections are separated by 6.4" 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 | Gaia DR3 391744074446299264 | 00:29:54.07 +50:11:00.6 (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 22.1516* 00 29 53.44 +50 11 02.4 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391744074446299264,2461093.6516,12.23,0.05,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 391744074446299264 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:53.44 +50:11:02.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.29 00:29:38.30 +42:09:08.4
118.61979 -20.53682 galactic And Second-epoch detections are separated by 6.0" and 4.2 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 varaible 381946291968937088 | 00:29:39.50 +42:09:15.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 29 38.30 +42 09 08.4 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 varaible 381946291968937088,2461093.6516,12.29,0.05,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 varaible 381946291968937088 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:38.30 +42:09:08.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 34 40.69 +50 22 02.5 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
T-Cas0-02113,2461093.6516,12.38,0.05,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
T-Cas0-02113 20260222.1516 12.38CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:40.69 +50:22:02.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 25 55.21 +49 48 43.2 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394632315394918784,2461093.6516,12.26,0.05,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 394632315394918784 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:25:55.21 +49:48:43.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.40 00:28:45.96 +49:15:40.7
119.13215 -13.44310 galactic Cas Second-epoch detections are separated by 3.3" 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 391228437852372480 | 00:28:45.41 +49:15:50.2 (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 22.1516* 00 28 45.96 +49 15 40.7 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391228437852372480,2461093.6516,12.40,0.05,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 391228437852372480 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:45.96 +49:15:40.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.41 00:39:53.15 +50:41:16.4
121.06082 -12.14189 galactic Cas Second-epoch detections are separated by 4.2" 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 | Gaia DR3 415602995732830848 | 00:39:53.92 +50:41:09.5 (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 22.1516* 00 39 53.15 +50 41 16.4 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415602995732830848,2461093.6516,12.41,0.05,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 415602995732830848 20260222.1516 12.41CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:53.15 +50:41:16.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 43 01.54 +51 05 22.7 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415263693316953088,2461093.6516,12.39,0.05,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 415263693316953088 20260222.1516 12.39CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:01.54 +51:05:22.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.36 00:36:16.28 +49:53:12.7
120.42663 -12.91110 galactic Cas Second-epoch detections are separated by 1.7" 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 391499909847350784 | 00:36:17.96 +49:53:04.2 (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 22.1516* 00 36 16.28 +49 53 12.7 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391499909847350784,2461093.6516,12.36,0.05,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 391499909847350784 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:16.28 +49:53:12.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.28 00:32:35.02 +50:01:53.6
119.82981 -12.72660 galactic Cas Second-epoch detections are separated by 1.7" and 5.1 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 391685731610882432 | 00:32:36.28 +50:01:59.1 (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 22.1516* 00 32 35.02 +50 01 53.6 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391685731610882432,2461093.6516,12.28,0.05,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 391685731610882432 20260222.1516 12.28CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:35.02 +50:01:53.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.35 00:28:48.90 +43:56:36.2
118.63464 -18.73952 galactic And Second-epoch detections are separated by 5.9" 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 varaible 382702167556886272 | 00:28:48.35 +43:57:01.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 28 48.90 +43 56 36.2 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 varaible 382702167556886272,2461093.6516,12.35,0.05,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 varaible 382702167556886272 20260222.1516 12.35CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:48.90 +43:56:36.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.34 00:27:29.41 +48:06:06.0
118.80472 -14.57808 galactic Cas Second-epoch detections are separated by 4.4" 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 | ATO J006.8780+48.1097 | 00:27:30.73 +48:06:35.0 (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 22.1516* 00 27 29.41 +48 06 06.0 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.8780+48.1097,2461093.6516,12.34,0.05,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
ATO J006.8780+48.1097 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:29.41 +48:06:06.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.29 00:28:37.06 +46:18:09.9
118.82698 -16.38703 galactic And Second-epoch detections are separated by 5.2" 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 389307831556379008 | 00:28:38.15 +46:18:13.4 (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 22.1516* 00 28 37.06 +46 18 09.9 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 389307831556379008,2461093.6516,12.29,0.05,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 389307831556379008 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:37.06 +46:18:09.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.22 00:46:52.35 +49:51:39.6
122.17681 -13.00406 galactic Cas Second-epoch detections are separated by 6.0" and 4.4 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 414568492729560320 | 00:46:53.28 +49:51:37.3 (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 22.1516* 00 46 52.35 +49 51 39.6 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414568492729560320,2461093.6516,12.22,0.05,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 414568492729560320 20260222.1516 12.22CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:46:52.35 +49:51:39.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.30 00:29:25.74 +49:41:21.6
119.28147 -13.02635 galactic Cas Second-epoch detections are separated by 6.4" and 5.0 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 391614263356154624 | 00:29:25.65 +49:41:13.8 (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 22.1516* 00 29 25.74 +49 41 21.6 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391614263356154624,2461093.6516,12.30,0.05,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 391614263356154624 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:25.74 +49:41:21.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.36 00:27:06.50 +49:21:19.4
118.86469 -13.32413 galactic Cas Second-epoch detections are separated by 1.3" and 5.1 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 391239432968429952 | 00:27:07.23 +49:21:32.3 (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 22.1516* 00 27 06.50 +49 21 19.4 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391239432968429952,2461093.6516,12.36,0.05,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 391239432968429952 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:06.50 +49:21:19.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.38 00:27:59.35 +50:27:49.0
119.11736 -12.23438 galactic Cas Second-epoch detections are separated by 5.3" and 5.3 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 J006.9988+50.4715 | 00:28:00.34 +50:27:39.5 (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 22.1516* 00 27 59.35 +50 27 49.0 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.9988+50.4715,2461093.6516,12.38,0.05,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
ATO J006.9988+50.4715 20260222.1516 12.38CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:59.35 +50:27:49.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.60 00:42:50.51 +44:36:28.4
121.32122 -18.23697 galactic And Second-epoch detections are separated by 4.4" 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 varaible 387998893025008512 | 00:42:49.46 +44:37:07.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 42 50.51 +44 36 28.4 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 varaible 387998893025008512,2461093.6516,12.60,0.05,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
Gaia DR3 varaible 387998893025008512 20260222.1516 12.60CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:50.51 +44:36:28.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.41 00:30:45.47 +45:18:50.6
119.12418 -17.40474 galactic And Second-epoch detections are separated by 7.9" 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 varaible 388704027874095104 | 00:30:46.09 +45:19:04.3 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 30 45.47 +45 18 50.6 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 varaible 388704027874095104,2461093.6516,12.41,0.05,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 varaible 388704027874095104 20260222.1516 12.41CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:45.47 +45:18:50.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.45 00:36:25.68 +45:37:21.6
120.18601 -17.16904 galactic And Second-epoch detections are separated by 4.1" 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 J009.1104+45.6268 | 00:36:26.50 +45:37:36.7 (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 22.1516* 00 36 25.68 +45 37 21.6 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
ATO J009.1104+45.6268,2461093.6516,12.45,0.05,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
ATO J009.1104+45.6268 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:25.68 +45:37:21.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.38 00:27:08.87 +49:17:55.6
118.86564 -13.38110 galactic Cas Second-epoch detections are separated by 5.0" and 5.3 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 391237680621781888 | 00:27:07.88 +49:17:40.9 (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 22.1516* 00 27 08.87 +49 17 55.6 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391237680621781888,2461093.6516,12.38,0.05,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 391237680621781888 20260222.1516 12.38CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:08.87 +49:17:55.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.44 00:26:33.82 +49:33:37.5
118.79484 -13.11142 galactic Cas Second-epoch detections are separated by 3.7" 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 394250239403705600 | 00:26:34.34 +49:33:41.4 (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 22.1516* 00 26 33.82 +49 33 37.5 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394250239403705600,2461093.6516,12.44,0.05,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 394250239403705600 20260222.1516 12.44CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:33.82 +49:33:37.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.42 00:26:03.00 +50:33:43.8
118.81323 -12.10644 galactic Cas Second-epoch detections are separated by 6.4" and 5.3 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 394678941559816320 | 00:26:04.27 +50:33:40.4 (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 22.1516* 00 26 03.00 +50 33 43.8 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394678941559816320,2461093.6516,12.42,0.05,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 394678941559816320 20260222.1516 12.42CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:03.00 +50:33:43.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.59 00:51:20.35 +44:10:03.3
122.91322 -18.70416 galactic And Second-epoch detections are separated by 2.0" 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 | Gaia DR3 varaible 375965120512652160 | 00:51:20.57 +44:09:32.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 51 20.35 +44 10 03.3 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 varaible 375965120512652160,2461093.6516,12.59,0.05,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 varaible 375965120512652160 20260222.1516 12.59CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:51:20.35 +44:10:03.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.53 00:38:19.68 +50:40:00.1
120.80762 -12.15097 galactic Cas Second-epoch detections are separated by 2.8" 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 415523727818379392 | 00:38:20.47 +50:39:58.1 (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 22.1516* 00 38 19.68 +50 40 00.1 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415523727818379392,2461093.6516,12.53,0.05,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 415523727818379392 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:19.68 +50:40:00.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.45 00:32:45.06 +49:39:07.0
119.82832 -13.10716 galactic Cas Second-epoch detections are separated by 6.3" 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 391577498432345728 | 00:32:47.73 +49:39:17.9 (Gaia DR3) | RRC (local) | (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 22.1516* 00 32 45.06 +49 39 07.0 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391577498432345728,2461093.6516,12.45,0.05,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 391577498432345728 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:45.06 +49:39:07.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.50 00:42:09.80 +50:45:46.9
121.43232 -12.08171 galactic Cas Second-epoch detections are separated by 1.7" and 5.3 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 J010.5572+50.7645 | 00:42:11.46 +50:45:55.0 (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 22.1516* 00 42 09.80 +50 45 46.9 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J010.5572+50.7645,2461093.6516,12.50,0.05,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
ATO J010.5572+50.7645 20260222.1516 12.50CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:09.80 +50:45:46.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.46 00:30:23.89 +50:09:25.7
119.48191 -12.57362 galactic Cas Second-epoch detections are separated by 4.0" and 4.7 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 391696451848937728 | 00:30:24.18 +50:09:19.2 (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 22.1516* 00 30 23.89 +50 09 25.7 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391696451848937728,2461093.6516,12.46,0.05,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 391696451848937728 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:23.89 +50:09:25.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.51 00:42:38.98 +46:09:02.8
121.34309 -16.69386 galactic And Second-epoch detections are separated by 8.1" 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 | ATO J010.6708+46.1471 | 00:42:37.83 +46:09:22.7 (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 22.1516* 00 42 38.98 +46 09 02.8 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 J010.6708+46.1471,2461093.6516,12.51,0.05,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
ATO J010.6708+46.1471 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:38.98 +46:09:02.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.54 00:33:43.39 +49:45:58.5
119.99774 -13.00455 galactic Cas 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 J008.4418+49.7694 | 00:33:46.05 +49:46:09.9 (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 22.1516* 00 33 43.39 +49 45 58.5 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J008.4418+49.7694,2461093.6516,12.54,0.05,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 J008.4418+49.7694 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:43.39 +49:45:58.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.57 00:42:03.89 +50:21:14.9
121.40082 -12.48974 galactic Cas Second-epoch detections are separated by 2.4" 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 414841755729732736 | 00:42:03.98 +50:20:58.7 (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 22.1516* 00 42 03.89 +50 21 14.9 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414841755729732736,2461093.6516,12.57,0.05,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 414841755729732736 20260222.1516 12.57CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:03.89 +50:21:14.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 32 30.81 +50 25 45.1 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391716071259718272,2461093.6516,12.48,0.05,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 391716071259718272 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:30.81 +50:25:45.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 31 01.26 +47 46 46.6 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6516,12.49,0.05,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
VARIABLE_NAME 20260222.1516 12.49CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:01.26 +47:46:46.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.55 00:29:14.34 +50:34:30.0
119.33009 -12.14144 galactic Cas Second-epoch detections are separated by 7.3" 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 391759433252132096 | 00:29:16.34 +50:34:27.8 (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 22.1516* 00 29 14.34 +50 34 30.0 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391759433252132096,2461093.6516,12.55,0.05,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 391759433252132096 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:14.34 +50:34:30.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.73 00:34:06.37 +43:14:12.9
119.58400 -19.52214 galactic And Second-epoch detections are separated by 4.6" 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 J008.5259+43.2401 | 00:34:06.23 +43:14:24.5 (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 22.1516* 00 34 06.37 +43 14 12.9 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
ATO J008.5259+43.2401,2461093.6516,12.73,0.05,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
ATO J008.5259+43.2401 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:06.37 +43:14:12.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.54 00:29:48.22 +44:49:04.6
118.90321 -17.88451 galactic And Second-epoch detections are separated by 4.2" 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 varaible 388760961960886272 | 00:29:51.12 +44:48:56.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 29 48.22 +44 49 04.6 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 varaible 388760961960886272,2461093.6516,12.54,0.05,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
Gaia DR3 varaible 388760961960886272 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:48.22 +44:49:04.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.77 00:43:04.15 +51:04:00.3
121.58903 -11.78318 galactic Cas Second-epoch detections are separated by 2.5" and 5.1 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 415251804847489792 | 00:43:04.57 +51:03:53.8 (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 22.1516* 00 43 04.15 +51 04 00.3 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415251804847489792,2461093.6516,12.77,0.05,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 415251804847489792 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:04.15 +51:04:00.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.56 00:30:17.47 +50:24:00.2
119.48531 -12.33012 galactic Cas Second-epoch detections are separated by 4.8" 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 391752385204645632 | 00:30:18.45 +50:23:55.1 (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 22.1516* 00 30 17.47 +50 24 00.2 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391752385204645632,2461093.6516,12.56,0.05,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 391752385204645632 20260222.1516 12.56CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:17.47 +50:24:00.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.61 00:30:53.38 +47:32:54.7
119.34168 -15.17993 galactic Cas Second-epoch detections are separated by 7.3" 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 390973862254336384 | 00:30:54.85 +47:33:04.5 (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 22.1516* 00 30 53.38 +47 32 54.7 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390973862254336384,2461093.6516,12.61,0.05,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 390973862254336384 20260222.1516 12.61CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:53.38 +47:32:54.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.56 00:26:55.34 +50:42:07.9
118.96814 -11.98078 galactic Cas Second-epoch detections are separated by 6.1" and 3.6 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 394771888951158656 | 00:26:56.90 +50:42:03.7 (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 22.1516* 00 26 55.34 +50 42 07.9 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394771888951158656,2461093.6516,12.56,0.05,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 394771888951158656 20260222.1516 12.56CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:55.34 +50:42:07.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.62 00:27:10.48 +49:24:48.3
118.88150 -13.26742 galactic Cas Second-epoch detections are separated by 2.9" 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 391240017084137216 | 00:27:10.14 +49:25:05.0 (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 22.1516* 00 27 10.48 +49 24 48.3 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391240017084137216,2461093.6516,12.62,0.05,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 391240017084137216 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:10.48 +49:24:48.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.65 00:26:22.18 +50:49:08.2
118.89096 -11.85601 galactic Cas Second-epoch detections are separated by 7.6" 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 394782059433673984 | 00:26:22.97 +50:48:59.8 (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 22.1516* 00 26 22.18 +50 49 08.2 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394782059433673984,2461093.6516,12.65,0.05,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 394782059433673984 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:22.18 +50:49:08.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.72 00:40:39.37 +50:04:30.0
121.15860 -12.75962 galactic Cas Second-epoch detections are separated by 4.0" 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 | Gaia DR3 414741390933380224 | 00:40:39.58 +50:04:18.9 (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 22.1516* 00 40 39.37 +50 04 30.0 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414741390933380224,2461093.6516,12.72,0.05,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 414741390933380224 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:39.37 +50:04:30.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 38 24.31 +50 36 29.7 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415520257482616448,2461093.6516,12.77,0.05,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 415520257482616448 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:24.31 +50:36:29.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.66 00:35:25.45 +50:14:35.3
120.31017 -12.54707 galactic Cas Second-epoch detections are separated by 2.5" 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 391525271628803328 | 00:35:25.63 +50:14:16.9 (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 22.1516* 00 35 25.45 +50 14 35.3 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391525271628803328,2461093.6516,12.66,0.05,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 391525271628803328 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:25.45 +50:14:35.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.65 00:28:47.38 +50:31:19.7
119.25255 -12.18774 galactic Cas Second-epoch detections are separated by 5.5" 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 | Gaia DR3 391769328856426752 | 00:28:48.06 +50:31:12.8 (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 22.1516* 00 28 47.38 +50 31 19.7 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391769328856426752,2461093.6516,12.65,0.05,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 391769328856426752 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:47.38 +50:31:19.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.71 00:26:39.13 +50:15:24.8
118.87984 -12.41975 galactic Cas Second-epoch detections are separated by 6.1" and 5.3 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 J006.6601+50.2514 | 00:26:40.06 +50:15:11.6 (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 22.1516* 00 26 39.13 +50 15 24.8 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.6601+50.2514,2461093.6516,12.71,0.05,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
ATO J006.6601+50.2514 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:39.13 +50:15:24.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.67 00:32:49.84 +49:47:49.1
119.85255 -12.96349 galactic Cas Second-epoch detections are separated by 5.9" and 4.6 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 | Large-amplitude variable Gaia DR2 391673740059458304 | 00:32:51.37 +49:47:49.5 (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 22.1516* 00 32 49.84 +49 47 49.1 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 391673740059458304,2461093.6516,12.67,0.05,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
Large-amplitude variable Gaia DR2 391673740059458304 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:49.84 +49:47:49.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.70 00:36:38.47 +42:10:48.9
120.00406 -20.60736 galactic And Second-epoch detections are separated by 6.7" 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 varaible 381515382194812416 | 00:36:40.83 +42:10:29.7 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 36 38.47 +42 10 48.9 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 varaible 381515382194812416,2461093.6516,12.70,0.05,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 varaible 381515382194812416 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:38.47 +42:10:48.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.82 00:39:19.76 +49:52:02.7
120.93029 -12.95727 galactic Cas Second-epoch detections are separated by 5.5" and 5.0 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 415459092849506048 | 00:39:20.93 +49:52:01.4 (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 22.1516* 00 39 19.76 +49 52 02.7 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415459092849506048,2461093.6516,12.82,0.05,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 415459092849506048 20260222.1516 12.82CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:39:19.76 +49:52:02.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.71 00:33:54.83 +50:30:03.4
120.08172 -12.27380 galactic Cas Second-epoch detections are separated by 1.8" and 5.1 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 415738579260650240 | 00:33:56.42 +50:30:03.5 (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 22.1516* 00 33 54.83 +50 30 03.4 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415738579260650240,2461093.6516,12.71,0.05,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 415738579260650240 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:54.83 +50:30:03.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.80 00:30:47.73 +49:36:54.7
119.50125 -13.11900 galactic Cas Second-epoch detections are separated by 1.9" 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 391585946631719552 | 00:30:48.81 +49:37:02.0 (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 22.1516* 00 30 47.73 +49 36 54.7 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391585946631719552,2461093.6516,12.80,0.05,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 391585946631719552 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:47.73 +49:36:54.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.83 00:35:57.52 +44:26:05.3
120.02162 -18.34946 galactic And Second-epoch detections are separated by 3.7" 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 varaible 387834000640608256 | 00:35:58.16 +44:26:20.1 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 35 57.52 +44 26 05.3 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 varaible 387834000640608256,2461093.6516,12.83,0.05,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 varaible 387834000640608256 20260222.1516 12.83CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:57.52 +44:26:05.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.84 00:38:45.82 +43:18:53.7
120.48676 -19.49665 galactic And Second-epoch detections are separated by 2.1" 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 | ATO J009.6958+43.3136 | 00:38:47.19 +43:18:38.9 (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 22.1516* 00 38 45.82 +43 18 53.7 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
ATO J009.6958+43.3136,2461093.6516,12.84,0.05,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
ATO J009.6958+43.3136 20260222.1516 12.84CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:45.82 +43:18:53.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.72 00:25:46.69 +49:53:38.0
118.69962 -12.76688 galactic Cas Second-epoch detections are separated by 6.4" 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 394633075607962112 | 00:25:47.86 +49:53:30.3 (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 22.1516* 00 25 46.69 +49 53 38.0 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394633075607962112,2461093.6516,12.72,0.05,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 394633075607962112 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:25:46.69 +49:53:38.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.82 00:31:56.93 +49:43:55.5
119.70178 -13.01739 galactic Cas Second-epoch detections are separated by 3.0" 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 J007.9878+49.7344 | 00:31:58.17 +49:43:58.3 (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 22.1516* 00 31 56.93 +49 43 55.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J007.9878+49.7344,2461093.6516,12.82,0.05,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
ATO J007.9878+49.7344 20260222.1516 12.82CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:31:56.93 +49:43:55.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.79 00:34:22.56 +49:51:07.5
120.11165 -12.92621 galactic Cas Second-epoch detections are separated by 5.7" 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 | Large-amplitude variable Gaia DR2 391489743662740992 | 00:34:23.23 +49:51:03.0 (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)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 34 22.56 +49 51 07.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 391489743662740992,2461093.6516,12.79,0.05,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
Large-amplitude variable Gaia DR2 391489743662740992 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:22.56 +49:51:07.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.71 00:26:47.68 +48:10:38.5
118.69303 -14.49146 galactic Cas Second-epoch detections are separated by 1.9" and 4.5 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 391060654951793024 | 00:26:49.26 +48:10:38.4 (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 22.1516* 00 26 47.68 +48 10 38.5 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391060654951793024,2461093.6516,12.71,0.05,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 391060654951793024 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:47.68 +48:10:38.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.77 00:26:48.36 +48:10:42.3
118.69508 -14.49059 galactic Cas Second-epoch detections are separated by 4.5" 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 391060654951793024 | 00:26:49.26 +48:10:38.4 (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 22.1516* 00 26 48.36 +48 10 42.3 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391060654951793024,2461093.6516,12.77,0.05,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 391060654951793024 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:48.36 +48:10:42.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.85 00:32:17.11 +50:32:02.5
119.81996 -12.22196 galactic Cas Second-epoch detections are separated by 3.5" and 5.1 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 391734556798920320 | 00:32:18.01 +50:31:58.9 (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 22.1516* 00 32 17.11 +50 32 02.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391734556798920320,2461093.6516,12.85,0.05,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 391734556798920320 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:17.11 +50:32:02.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.73 00:30:17.55 +44:55:50.5
119.00416 -17.77973 galactic And Second-epoch detections are separated by 8.6" 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 | ATO J007.5800+44.9379 | 00:30:18.71 +44:56:04.4 (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 22.1516* 00 30 17.55 +44 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
ATO J007.5800+44.9379,2461093.6516,12.73,0.05,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
ATO J007.5800+44.9379 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:17.55 +44:55:50.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.76 00:27:52.04 +49:20:06.7
118.98918 -13.35603 galactic Cas Second-epoch detections are separated by 0.6" and 5.1 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 391235825196083968 | 00:27:51.41 +49:20:07.9 (Gaia DR3) | ROT (local) | (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 22.1516* 00 27 52.04 +49 20 06.7 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391235825196083968,2461093.6516,12.76,0.05,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 391235825196083968 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:52.04 +49:20:06.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.87 00:27:31.27 +47:36:58.9
118.76190 -15.06165 galactic Cas 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 | Gaia DR3 389533197080919168 | 00:27:31.87 +47:37:16.4 (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 22.1516* 00 27 31.27 +47 36 58.9 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389533197080919168,2461093.6516,12.87,0.05,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 389533197080919168 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:31.27 +47:36:58.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.99 00:33:57.83 +49:37:29.4
120.02742 -13.14834 galactic Cas Second-epoch detections are separated by 3.6" 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 | ATO J008.4995+49.6254 | 00:33:59.88 +49:37:31.6 (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 22.1516* 00 33 57.83 +49 37 29.4 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J008.4995+49.6254,2461093.6516,12.99,0.05,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 J008.4995+49.6254 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:57.83 +49:37:29.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.85 00:26:11.72 +50:49:43.5
118.86397 -11.84351 galactic Cas Second-epoch detections are separated by 8.9" 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 394782231232356992 | 00:26:12.27 +50:49:57.0 (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 22.1516* 00 26 11.72 +50 49 43.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394782231232356992,2461093.6516,12.85,0.05,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 394782231232356992 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:11.72 +50:49:43.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.87 00:32:27.85 +44:48:22.3
119.39637 -17.93526 galactic And Second-epoch detections are separated by 2.8" 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 varaible 388650422384900224 | 00:32:27.52 +44:48:45.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') J-Ks=0.817+/-0.073 (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 22.1516* 00 32 27.85 +44 48 22.3 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 varaible 388650422384900224,2461093.6516,12.87,0.05,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 varaible 388650422384900224 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:27.85 +44:48:22.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.82 00:28:33.50 +44:52:49.4
118.67824 -17.80231 galactic And Second-epoch detections are separated by 5.1" 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 | ATO J007.1460+44.8801 | 00:28:35.04 +44:52:48.4 (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 22.1516* 00 28 33.50 +44 52 49.4 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
ATO J007.1460+44.8801,2461093.6516,12.82,0.05,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
ATO J007.1460+44.8801 20260222.1516 12.82CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:33.50 +44:52:49.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.01 00:33:24.86 +41:45:46.1
119.33357 -20.98298 galactic And Second-epoch detections are separated by 5.9" 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 varaible 381867402009833088 | 00:33:25.73 +41:46:11.4 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 33 24.86 +41 45 46.1 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 varaible 381867402009833088,2461093.6516,13.01,0.05,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 varaible 381867402009833088 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:24.86 +41:45:46.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.87 00:32:39.56 +50:18:05.6
119.86288 -12.45826 galactic Cas Second-epoch detections are separated by 4.9" 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 391712978883318272 | 00:32:40.39 +50:17:58.8 (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 22.1516* 00 32 39.56 +50 18 05.6 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391712978883318272,2461093.6516,12.87,0.05,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 391712978883318272 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:39.56 +50:18:05.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.86 00:29:11.93 +45:39:08.5
118.87003 -17.04392 galactic And Second-epoch detections are separated by 6.2" and 5.1 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 varaible 388900561279597440 | 00:29:12.20 +45:39:20.2 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 29 11.93 +45 39 08.5 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 varaible 388900561279597440,2461093.6516,12.86,0.05,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
Gaia DR3 varaible 388900561279597440 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:11.93 +45:39:08.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.85 00:27:32.67 +49:57:23.8
118.99601 -12.73245 galactic Cas Second-epoch detections are separated by 2.6" and 4.5 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 391635291515859200 | 00:27:33.67 +49:57:23.1 (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 22.1516* 00 27 32.67 +49 57 23.8 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391635291515859200,2461093.6516,12.85,0.05,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 391635291515859200 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:32.67 +49:57:23.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.99 00:27:43.85 +49:51:46.5
119.01754 -12.82856 galactic Cas Second-epoch detections are separated by 8.1" and 4.8 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 391630412433036288 | 00:27:42.96 +49:51:29.5 (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 22.1516* 00 27 43.85 +49 51 46.5 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391630412433036288,2461093.6516,12.99,0.05,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 391630412433036288 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:43.85 +49:51:46.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.88 00:34:24.44 +50:39:44.8
120.17301 -12.11805 galactic Cas Second-epoch detections are separated by 4.7" 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 415559427583971840 | 00:34:25.12 +50:39:43.3 (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 22.1516* 00 34 24.44 +50 39 44.8 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415559427583971840,2461093.6516,12.88,0.05,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 415559427583971840 20260222.1516 12.88CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:24.44 +50:39:44.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.91 00:27:06.77 +50:39:40.1
118.99478 -12.02456 galactic Cas Second-epoch detections are separated by 8.0" 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 394771510994048384 | 00:27:07.55 +50:39:29.4 (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 22.1516* 00 27 06.77 +50 39 40.1 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394771510994048384,2461093.6516,12.91,0.05,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
Gaia DR3 394771510994048384 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:06.77 +50:39:40.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.90 00:32:17.53 +50:32:04.4
119.82114 -12.22152 galactic Cas Second-epoch detections are separated by 1.9" and 5.0 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 391734556798920320 | 00:32:18.01 +50:31:58.9 (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 22.1516* 00 32 17.53 +50 32 04.4 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391734556798920320,2461093.6516,12.90,0.05,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
Gaia DR3 391734556798920320 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:17.53 +50:32:04.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.92 00:29:26.36 +49:15:10.3
119.24389 -13.46129 galactic Cas Second-epoch detections are separated by 5.0" 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 | Gaia DR3 391226303249926016 | 00:29:26.10 +49:15:19.1 (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 22.1516* 00 29 26.36 +49 15 10.3 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391226303249926016,2461093.6516,12.92,0.05,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 391226303249926016 20260222.1516 12.92CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:26.36 +49:15:10.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.98 00:26:22.26 +49:05:47.5
118.71532 -13.56988 galactic Cas Second-epoch detections are separated by 4.7" 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 | ATO J006.5873+49.0937 | 00:26:23.62 +49:05:43.4 (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 22.1516* 00 26 22.26 +49 05 47.5 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.5873+49.0937,2461093.6516,12.98,0.05,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
ATO J006.5873+49.0937 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:22.26 +49:05:47.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.48 01:55:41.06 +50:00:11.6
133.38965 -11.55948 galactic Per Second-epoch detections are separated by 0.3" 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 | target | 01:55:41.06 +50:00:11.6 (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 22.1516* 01 55 41.06 +50 00 11.6 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
target,2461093.6516,13.48,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:41.06 +50:00:11.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.97 00:33:53.67 +50:00:13.5
120.04307 -12.76957 galactic Cas Second-epoch detections are separated by 1.7" and 5.3 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 391495584818219264 | 00:33:54.37 +50:00:10.5 (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 22.1516* 00 33 53.67 +50 00 13.5 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391495584818219264,2461093.6516,12.97,0.05,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 391495584818219264 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:53.67 +50:00:13.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.06 00:42:59.68 +50:33:07.4
121.55944 -12.29719 galactic Cas Second-epoch detections are separated by 3.2" and 4.8 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 414839625425894016 | 00:43:00.04 +50:33:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.358+/-0.067 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 42 59.68 +50 33 07.4 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414839625425894016,2461093.6516,13.06,0.05,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 414839625425894016 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:42:59.68 +50:33:07.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.92 00:34:43.74 +43:16:57.3
119.70740 -19.48453 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 varaible 382428427818316544 | 00:34:43.88 +43:17:11.0 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 34 43.74 +43 16 57.3 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 varaible 382428427818316544,2461093.6516,12.92,0.05,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 varaible 382428427818316544 20260222.1516 12.92CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:43.74 +43:16:57.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.09 00:30:06.90 +49:21:47.8
119.36649 -13.36080 galactic Cas Second-epoch detections are separated by 7.9" and 3.8 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 391555503903542912 | 00:30:08.14 +49:21:57.7 (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 22.1516* 00 30 06.90 +49 21 47.8 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391555503903542912,2461093.6516,13.09,0.05,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 391555503903542912 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:06.90 +49:21:47.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 27 17.58 +48 55 28.3 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391200980125266176,2461093.6516,12.96,0.05,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 391200980125266176 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:17.58 +48:55:28.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.96 00:29:40.13 +48:41:42.0
119.23235 -14.02031 galactic Cas Second-epoch detections are separated by 5.9" and 4.7 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 391141400336403584 | 00:29:41.37 +48:41:39.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.330+/-0.065 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 29 40.13 +48 41 42.0 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391141400336403584,2461093.6516,12.96,0.05,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 391141400336403584 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:40.13 +48:41:42.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.07 00:27:31.22 +46:55:30.7
118.69281 -15.74960 galactic Cas Second-epoch detections are separated by 3.3" and 5.3 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 389396307882472704 | 00:27:32.44 +46:55:30.0 (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 22.1516* 00 27 31.22 +46 55 30.7 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389396307882472704,2461093.6516,13.07,0.05,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 389396307882472704 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:31.22 +46:55:30.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.00 00:32:44.96 +47:06:11.4
119.63109 -15.64877 galactic Cas Second-epoch detections are separated by 1.4" and 5.3 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 389273364441206912 | 00:32:46.40 +47:05:57.9 (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 22.1516* 00 32 44.96 +47 06 11.4 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 389273364441206912,2461093.6516,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 389273364441206912 20260222.1516 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:44.96 +47:06:11.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.05 00:26:35.88 +48:52:42.5
118.73112 -13.79056 galactic Cas Second-epoch detections are separated by 3.3" and 5.1 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 391202187012124928 | 00:26:36.67 +48:52:44.6 (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 22.1516* 00 26 35.88 +48 52 42.5 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391202187012124928,2461093.6516,13.05,0.05,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 391202187012124928 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:35.88 +48:52:42.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.04 00:28:50.50 +50:45:50.7
119.28313 -11.94751 galactic Cas Second-epoch detections are separated by 7.3" 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 | ATO J007.2198+50.7649 | 00:28:51.06 +50:45:41.7 (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 22.1516* 00 28 50.50 +50 45 50.7 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J007.2198+50.7649,2461093.6516,13.04,0.05,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
ATO J007.2198+50.7649 20260222.1516 13.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:50.50 +50:45:50.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.10 00:34:32.15 +43:30:48.6
119.68721 -19.25174 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 varaible 388437117129639552 | 00:34:32.47 +43:31:03.8 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 34 32.15 +43 30 48.6 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 varaible 388437117129639552,2461093.6516,13.10,0.05,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 varaible 388437117129639552 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:34:32.15 +43:30:48.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.96 00:27:55.45 +50:17:57.2
119.09112 -12.39709 galactic Cas Second-epoch detections are separated by 3.5" and 5.0 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 391667310493026304 | 00:27:56.30 +50:17:49.4 (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 22.1516* 00 27 55.45 +50 17 57.2 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391667310493026304,2461093.6516,12.96,0.05,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 391667310493026304 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:55.45 +50:17:57.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.18 00:36:52.19 +49:27:44.5
120.50006 -13.34059 galactic Cas Second-epoch detections are separated by 3.7" 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 | ATO J009.2175+49.4637 | 00:36:53.12 +49:27:43.0 (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 22.1516* 00 36 52.19 +49 27 44.5 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J009.2175+49.4637,2461093.6516,13.18,0.05,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
ATO J009.2175+49.4637 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:36:52.19 +49:27:44.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.05 00:27:26.86 +48:32:01.5
118.84024 -14.14731 galactic Cas Second-epoch detections are separated by 4.0" and 5.3 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 J006.8711+48.5376 | 00:27:27.59 +48:31:57.5 (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 22.1516* 00 27 26.86 +48 32 01.5 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.8711+48.5376,2461093.6516,13.05,0.05,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 J006.8711+48.5376 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:26.86 +48:32:01.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.14 00:27:44.21 +50:49:28.8
119.11113 -11.87117 galactic Cas Second-epoch detections are separated by 2.4" and 4.5 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 J006.9427+50.8280 | 00:27:45.30 +50:49:27.2 (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 22.1516* 00 27 44.21 +50 49 28.8 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J006.9427+50.8280,2461093.6516,13.14,0.05,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
ATO J006.9427+50.8280 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:27:44.21 +50:49:28.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 32 55.99 +47 12 34.8 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 390775439062245504,2461093.6516,13.12,0.05,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 390775439062245504 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:55.99 +47:12:34.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.11 00:26:03.54 +49:35:56.5
118.71523 -13.06482 galactic Cas Second-epoch detections are separated by 6.5" 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 394250926598652928 | 00:26:05.23 +49:35:57.0 (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 22.1516* 00 26 03.54 +49 35 56.5 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394250926598652928,2461093.6516,13.11,0.05,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 394250926598652928 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:26:03.54 +49:35:56.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.11 00:40:15.10 +50:56:11.3
121.13131 -11.89616 galactic Cas Second-epoch detections are separated by 2.0" and 5.0 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 | Large-amplitude variable Gaia DR2 415613750328497024 | 00:40:16.45 +50:56:11.1 (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 22.1516* 00 40 15.10 +50 56 11.3 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 415613750328497024,2461093.6516,13.11,0.05,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
Large-amplitude variable Gaia DR2 415613750328497024 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:40:15.10 +50:56:11.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.22 00:30:24.08 +41:20:21.0
118.69415 -21.35942 galactic And Second-epoch detections are separated by 3.0" 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 varaible 381839463245987584 | 00:30:24.30 +41:20:38.6 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known')
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 00 30 24.08 +41 20 21.0 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 varaible 381839463245987584,2461093.6516,13.22,0.05,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 varaible 381839463245987584 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:24.08 +41:20:21.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.18 00:28:14.64 +48:43:14.6
118.99345 -13.97358 galactic Cas Second-epoch detections are separated by 3.2" and 5.1 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 391185110222477696 | 00:28:15.65 +48:43:17.0 (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 22.1516* 00 28 14.64 +48 43 14.6 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391185110222477696,2461093.6516,13.18,0.05,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 391185110222477696 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:28:14.64 +48:43:14.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 33 54.10 +47 12 58.0 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6516,13.24,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:33:54.10 +47:12:58.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.21 00:25:35.00 +50:09:14.2
118.69498 -12.50499 galactic Cas Second-epoch detections are separated by 5.1" and 4.8 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 394644414321556224 | 00:25:36.69 +50:09:18.0 (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 22.1516* 00 25 35.00 +50 09 14.2 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 394644414321556224,2461093.6516,13.21,0.05,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 394644414321556224 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:25:35.00 +50:09:14.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.99 00:30:08.26 +49:34:49.0
119.38919 -13.14490 galactic Cas Second-epoch detections are separated by 7.3" 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 391565846184775808 | 00:30:09.36 +49:34:52.6 (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 22.1516* 00 30 08.26 +49 34 49.0 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391565846184775808,2461093.6516,12.99,0.05,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 391565846184775808 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:30:08.26 +49:34:49.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.81 00:38:56.24 +50:58:31.5
120.92191 -11.84754 galactic Cas Second-epoch detections are separated by 2.1" 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 J009.7331+50.9805 | 00:38:57.12 +50:58:23.7 (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 22.1516* 00 38 56.24 +50 58 31.5 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J009.7331+50.9805,2461093.6516,11.81,0.05,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
ATO J009.7331+50.9805 20260222.1516 11.81CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:56.24 +50:58:31.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.59 00:54:54.46 +41:10:28.6
123.63460 -21.69240 galactic And Second-epoch detections are separated by 2.1" 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 | Gaia DR3 varaible 374319632641787008 | 00:54:54.14 +41:10:38.9 (Gaia DR3) | | 2022yCat.1358....0G | Gaia3var=NOT_AVAILABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') 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 22.1516* 00 54 54.46 +41 10 28.6 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 varaible 374319632641787008,2461093.6516,12.59,0.05,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 varaible 374319632641787008 20260222.1516 12.59CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:54:54.46 +41:10:28.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.01 01:20:28.68 +43:52:02.2
128.45124 -18.69304 galactic And Second-epoch detections are separated by 5.5" and 5.0 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 | 01:20:28.68 +43:52:02.2 (user input) | T | P | (position from user input) 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 22.1516* 01 20 28.68 +43 52 02.2 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
target,2461093.6516,13.01,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:20:28.68 +43:52:02.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 28 03.50 +49 29 53.6 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
NSVS J0128039+492957,2461093.6516,13.30,0.05,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
NSVS J0128039+492957 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:28:03.50 +49:29:53.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 16 04.64 +50 11 40.0 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
V0417 And,2461093.6516,11.36,0.05,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
V0417 And 20260222.1516 11.36CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:16:04.64 +50:11:40.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 23 44.50 +49 24 07.3 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
target,2461093.6516,13.35,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:23:44.50 +49:24:07.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 17 55.72 +50 24 13.4 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
ASASSN-V J011755.51+502415.6,2461093.6516,11.83,0.05,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
ASASSN-V J011755.51+502415.6 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:17:55.72 +50:24:13.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 47 53.15 +48 30 44.7 9.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J004752.43+483046.8,2461093.6516,9.63,0.05,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
ASASSN-V J004752.43+483046.8 20260222.1516 9.63CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:47:53.15 +48:30:44.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 10 12.11 +50 22 50.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J0110118+502254,2461093.6516,12.12,0.05,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
NSVS J0110118+502254 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:10:12.11 +50:22:50.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 00 04.24 +48 40 23.8 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
ASASSN-V J010004.18+484027.5,2461093.6516,12.82,0.05,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
ASASSN-V J010004.18+484027.5 20260222.1516 12.82CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:00:04.24 +48:40:23.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 31 54.80 +46 49 07.2 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
NSVS J0131553+464908,2461093.6516,12.46,0.05,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
NSVS J0131553+464908 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:31:54.80 +46:49:07.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.86 00:29:25.84 +48:36:05.5
119.18352 -14.10998 galactic Cas Second-epoch detections are separated by 5.3" 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 | Gaia DR3 391133360157631488 | 00:29:26.71 +48:36:06.0 (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 22.1516* 00 29 25.84 +48 36 05.5 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391133360157631488,2461093.6516,12.86,0.05,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
Gaia DR3 391133360157631488 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:29:25.84 +48:36:05.5 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 49 14.16 +46 59 32.7 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J0049130+465947,2461093.6516,12.91,0.05,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
NSVS J0049130+465947 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:49:14.16 +46:59:32.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 16 57.43 +49 34 43.7 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
ASASSN-V J011657.52+493447.8,2461093.6516,12.33,0.05,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
ASASSN-V J011657.52+493447.8 20260222.1516 12.33CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:16:57.43 +49:34:43.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 17 29.78 +47 41 12.0 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
target,2461093.6516,13.11,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:17:29.78 +47:41:12.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.19 01:23:46.35 +47:16:25.4
128.60703 -15.24142 galactic And Second-epoch detections are separated by 3.6" 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 | target | 01:23:46.35 +47:16:25.4 (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 22.1516* 01 23 46.35 +47 16 25.4 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
target,2461093.6516,13.19,0.05,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
target 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:23:46.35 +47:16:25.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 56 40.47 +48 44 11.4 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J005639.96+484413.4,2461093.6516,12.63,0.05,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
ASASSN-V J005639.96+484413.4 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:56:40.47 +48:44:11.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 12 32.83 +50 51 24.3 13.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J011231.37+505132.9,2461093.6516,13.04,0.05,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
ZTF J011231.37+505132.9 20260222.1516 13.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:12:32.83 +50:51:24.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 20 54.65 +49 35 51.8 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
target,2461093.6516,13.03,0.05,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 20260222.1516 13.03CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:20:54.65 +49:35:51.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 11 45.37 +43 16 18.1 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
ASASSN-V J011145.39+431616.9,2461093.6516,12.30,0.05,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
ASASSN-V J011145.39+431616.9 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:11:45.37 +43:16:18.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 49 08.09 +48 12 50.7 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J004907.52+481253.8,2461093.6516,13.26,0.05,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
ASASSN-V J004907.52+481253.8 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:49:08.09 +48:12:50.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.50 00:32:18.61 +50:27:38.4
119.81832 -12.29541 galactic Cas Second-epoch detections are separated by 2.1" and 5.3 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 391716346137608064 | 00:32:19.68 +50:27:30.0 (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 22.1516* 00 32 18.61 +50 27 38.4 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391716346137608064,2461093.6516,12.50,0.05,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 391716346137608064 20260222.1516 12.50CV 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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:32:18.61 +50:27:38.4 ;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-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 38 53.25 +45 33 49.7 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
V0403 And,2461093.6516,12.34,0.05,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
V0403 And 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:38:53.25 +45:33:49.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 12.64 00:35:44.05 +50:33:08.7
120.38060 -12.24152 galactic Cas Second-epoch detections are separated by 1.3" 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 | ATO J008.9218+50.5419 | 00:35:44.23 +50:33:01.8 (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 22.1516* 00 35 44.05 +50 33 08.7 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J008.9218+50.5419,2461093.6516,12.64,0.05,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
ATO J008.9218+50.5419 20260222.1516 12.64CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:35:44.05 +50:33:08.7 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 57 28.45 +42 47 54.3 9.0 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
NSVS 3798741,2461093.6516,9.04,0.05,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
NSVS 3798741 20260222.1516 9.04CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:57:28.45 +42:47:54.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 24 25.24 +45 36 20.1 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 398044585309837696,2461093.6516,13.05,0.05,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 398044585309837696 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:24:25.24 +45:36:20.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 8.91 01:06:04.74 +49:51:20.0
125.35239 -12.94737 galactic Cas Second-epoch detections are separated by 0.3" 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 varaible 404200063720488448 | 01:06:04.55 +49:51:23.4 (Gaia DR3) | LPV (Gaia DR3) | 2022yCat.1358....0G | Gaia3var=VARIABLE Gaia DR3 varaible (the VSX policy as of July 2022 is to regard variables from Gaia DR3 as 'known') SpType: M8 1973AJ.....78..389V IRC +50026
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1516* 01 06 04.74 +49 51 20.0 8.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 varaible 404200063720488448,2461093.6516,8.91,0.05,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 varaible 404200063720488448 20260222.1516 8.91CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:06:04.74 +49:51:20.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.42 00:43:46.56 +51:02:35.7
121.70168 -11.81020 galactic Cas Second-epoch detections are separated by 6.2" and 4.5 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 415251014574107776 | 00:43:47.55 +51:02:34.5 (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 22.1516* 00 43 46.56 +51 02 35.7 11.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 415251014574107776,2461093.6516,11.42,0.05,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 415251014574107776 20260222.1516 11.42CV 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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:43:46.56 +51:02:35.7 ;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-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 14 22.24 +47 04 47.6 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
NSVS J0114223+470450,2461093.6516,11.81,0.05,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
NSVS J0114223+470450 20260222.1516 11.81CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:14:22.24 +47:04:47.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 51 23.98 +49 09 52.9 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 414478122321739392,2461093.6516,11.56,0.05,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 414478122321739392 20260222.1516 11.56CV 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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:51:23.98 +49:09:52.9 ;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-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 37 29.69 +47 55 39.9 10.6 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 3879840,2461093.6516,10.57,0.05,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
NSVS 3879840 20260222.1516 10.57CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:37:29.69 +47:55:39.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 26 55.54 +47 24 02.8 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
ASASSN-V J012655.73+472404.1,2461093.6516,12.92,0.05,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
ASASSN-V J012655.73+472404.1 20260222.1516 12.92CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:26:55.54 +47:24:02.8 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 36 40.37 +42 51 19.4 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
NSVS J0136406+425115,2461093.6516,11.55,0.05,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 J0136406+425115 20260222.1516 11.55CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:36:40.37 +42:51:19.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 11.27 01:22:04.52 +46:06:40.4
128.46004 -16.43141 galactic And Second-epoch detections are separated by 0.3" 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 398124471701427328 | 01:22:04.08 +46:06:45.6 (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 22.1516* 01 22 04.52 +46 06 40.4 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 398124471701427328,2461093.6516,11.27,0.05,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 398124471701427328 20260222.1516 11.27CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:22:04.52 +46:06:40.4 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 31 04.14 +47 34 41.3 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
NSVS J0131044+473443,2461093.6516,12.43,0.05,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
NSVS J0131044+473443 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:31:04.14 +47:34:41.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 54 27.34 +43 55 38.0 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
NSVS 3796573,2461093.6516,12.64,0.05,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
NSVS 3796573 20260222.1516 12.64CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:54:27.34 +43:55:38.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 00 48.10 +50 23 41.6 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 402976410357657984,2461093.6516,13.07,0.05,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 402976410357657984 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:00:48.10 +50:23:41.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1516 2461093.6516 13.66 01:35:12.12 +46:33:47.6
130.72048 -15.64563 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 J023.7964+46.5669 | 01:35:12.12 +46:33:47.6 (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 22.1516* 01 35 12.12 +46 33 47.6 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
ATO J023.7964+46.5669,2461093.6516,13.66,0.05,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 J023.7964+46.5669 20260222.1516 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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:35:12.12 +46:33:47.6 ;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-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 06 23.29 +47 20 01.6 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
ASASSN-V J010623.12+472003.1,2461093.6516,12.39,0.05,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
ASASSN-V J010623.12+472003.1 20260222.1516 12.39CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:06:23.29 +47:20:01.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 07 26.54 +45 36 35.6 8.1 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
EI And,2461093.6516,8.12,0.05,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
EI And 20260222.1516 8.12CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:07:26.54 +45:36:35.6 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 21 37.14 +43 32 51.2 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
NSVS J0121373+433248,2461093.6516,12.69,0.05,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
NSVS J0121373+433248 20260222.1516 12.69CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:21:37.14 +43:32:51.2 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 23 44.46 +45 52 03.1 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
ASASSN-V J012344.58+455203.3,2461093.6516,12.95,0.05,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
ASASSN-V J012344.58+455203.3 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:23:44.46 +45:52:03.1 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 00 21.25 +48 54 15.3 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 3761771,2461093.6516,13.36,0.05,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
NSVS 3761771 20260222.1516 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:00:21.25 +48:54:15.3 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 01 14 22.06 +49 58 28.9 10.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J011422.12+495833.6,2461093.6516,10.91,0.05,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
ASASSN-V J011422.12+495833.6 20260222.1516 10.91CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:14:22.06 +49:58:28.9 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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 22.1516* 00 57 04.39 +48 42 09.0 7.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KS Cas,2461093.6516,7.67,0.05,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
KS Cas 20260222.1516 7.67CV 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 00:57:04.39 +48:42:09.0 ;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-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20_00sec_-15_00C_LIGHT_0083_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png resample_wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20_00sec_-15_00C_LIGHT_0082_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: 2461032.71026414 23.12.2025 05:02:36.822 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
First image: 2461032.71026414 23.12.2025 05:02:36.822 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
Last image: 2461093.65189238 22.02.2026 03:38:33.502 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 149
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: 17 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): 22585
Objects passed selection criteria: 22510
Measurements per detected object (mean, median, min, max): 3.0 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 4.0 2 4
Average stars detected per image: 17951.5
Average stars matched: 17523 (97.613 %)
Memory usage VmPeak: 126932 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 Sun Feb 22 02:38:27 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: 2461032.71026414 23.12.2025 05:02:36.822 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
First image: 2461032.71026414 23.12.2025 05:02:36.822 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
Last image: 2461093.65189238 22.02.2026 03:38:33.502 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1403
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 158 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): 141406
Objects passed selection criteria: 141026
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 104956
Average stars matched: 100664 (95.9111 %)
Memory usage VmPeak: 1902764 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 Sun Feb 22 02:46:07 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-02-Q2b1x1
#######################################
########### Starting And-02-Q2b1x1 ###########
Processing And-02-Q2b1x1
server tau has sufficient free disk space available: 1057305 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1057305 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.png' -> 'transient_report/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits_preview.png'
And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
renamed 'And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.png' -> 'transient_report/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits_preview.png'
And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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= 577.5024
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 771.9064
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1492.4846
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 723.3944
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1494.2295
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 723.2200
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.58438
INFO: SECOND_EPOCH__SD_ratio= 0.000
----------------------------------------------
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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
SExtractor catalog cache: saved And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat to cache
SExtractor catalog cache: saved And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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: 2461093.65130784
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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits exists and is non-empty
Saving wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits to local_wcs_cache/
'wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits' -> 'local_wcs_cache/wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits'
wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits exists and is non-empty
Saving wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits to local_wcs_cache/
'wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits' -> 'local_wcs_cache/wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits'
wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits exists and is non-empty
Saving wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits to local_wcs_cache/
'wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits' -> 'local_wcs_cache/wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits'
wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits exists and is non-empty
Saving wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits to local_wcs_cache/
'wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits' -> 'local_wcs_cache/wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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 01:12:00.218 +45:59:53.67
Second-epoch image center 01:11:57.773 +46:00:02.51
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 01:12:00.218 +45:59:53.67
Second-epoch image center 01:12:01.103 +46:00:06.97
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 01:11:57.773 +46:00:02.51
Second-epoch second image center 01:12:01.103 +46:00:06.97
Angular distance between the image centers 0.00972 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits &> /tmp/tmp.5JppiX5XvM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits &> /tmp/tmp.1idtAZED8u
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits &> /tmp/tmp.7GDrQOpU7a
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits &> /tmp/tmp.cGu4aBcPvS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
Calibrating the magnitude scale
Found non-empty wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits and wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits and wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat
Found non-empty wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits and wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat
The reference image (wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits) and catalog (wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat) found
'wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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 11868 out of 24040 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.925462
a=0.000000 b=1.000000 c=22.925462
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 127 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
2.1 pix And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
3.8 pix And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
3.8 pix And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
Limiting magnitude estimates:
15.3 mag. And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
15.3 mag. And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
14.2 mag. And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
14.2 mag. And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.8 (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.5JppiX5XvM (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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits' -> 'wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
Checking if the catalog wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
WCS catalog name: wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2125, passed=24040
Got 24040 stars (including 21880 good ones) from the SExtractor catalog wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat
util/solve_plate_with_UCAC5 got 24040 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 936 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: 0.43"
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 936 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: 0.42"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits -region wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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.1idtAZED8u (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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits' -> 'wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
Checking if the catalog wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
WCS catalog name: wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2156, passed=23990
Got 23990 stars (including 21810 good ones) from the SExtractor catalog wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat
util/solve_plate_with_UCAC5 got 23990 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 937 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: 0.43"
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 937 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: 0.42"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits -region wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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.7GDrQOpU7a (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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
WCS-calibrated image found: wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
Checking if the catalog wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
WCS catalog name: wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1296, passed=12171
Got 12171 stars (including 10870 good ones) from the SExtractor catalog wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat
util/solve_plate_with_UCAC5 got 12171 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 926 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: 0.95"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.00"
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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.01"
Estimated accuracy of the plate solution: 1.08"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits -region wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.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.cGu4aBcPvS (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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
WCS-calibrated image found: wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
Checking if the catalog wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
WCS catalog name: wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1320, passed=12184
Got 12184 stars (including 10862 good ones) from the SExtractor catalog wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 12184 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 923 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: 0.97"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.02"
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 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.02"
Estimated accuracy of the plate solution: 1.10"
Excluding outliers - 917 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits -region wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out31456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31584.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__out31599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10177.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31527.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31596.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31615.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 60s
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: 31s
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Considering the candidate 31456_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31456_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:54.82 +42:33:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 4.333 382300502216005760 007.97911256821 +42.55703351893 9.9599 9.5222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31459_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31459_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:47.54 +51:02:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.28, MAG_FAINT_SEARCH_LIMIT=12.26)GAIADR2_OUTPUT=# 1.346 415251014574107776 010.94812972618 +51.04290497636 10.4256 10.0634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31460_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31460_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:50.34 +50:26:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)GAIADR2_OUTPUT=# 1.560 414612267036266496 011.96042983322 +50.43793003833 10.3721 9.9561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31461_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31461_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:48.56 +44:23:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 0.585 387796415383551104 009.95248960812 +44.39979847241 10.2082 9.7796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31463_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31463_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:31.48 +49:05:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 1.741 390613089298382592 010.88171754806 +49.08759443228 10.3149 9.8773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31465_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31465_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:29.70 +50:38:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 3.496 414981909102347136 012.37471217402 +50.63511667428 10.4484 10.0497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31466_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31466_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:45.96 +48:49:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 2.959 390545194455385984 009.94037651968 +48.81897472972 10.1694 9.7803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31467_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31467_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:06.55 +41:18:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.22, MAG_FAINT_SEARCH_LIMIT=12.20)GAIADR2_OUTPUT=# 3.323 369224049084752256 011.52831396319 +41.30887318038 10.1446 9.7516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31468_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31468_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31469_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31469_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:04.08 +43:58:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 2.975 387771740795374592 010.01796760584 +43.96891734028 10.1395 9.7088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31470_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31470_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:14.43 +49:18:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 1.400 391412193733783552 009.31065254405 +49.30870748566 9.9058 9.5950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31471_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31471_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31474_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31474_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:55.38 +48:43:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.998 390962970215059072 008.48123136879 +48.71976711288 9.9156 9.4628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31475_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31475_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31476_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31476_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:31.23 +41:50:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.96, MAG_FAINT_SEARCH_LIMIT=11.94)GAIADR2_OUTPUT=# 4.194 381349085363172864 010.13104123926 +41.83802721933 9.8349 9.1877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31477_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31477_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:18.29 +49:41:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.17, MAG_FAINT_SEARCH_LIMIT=12.15)GAIADR2_OUTPUT=# 0.819 414668994965012864 011.07604198974 +49.68996629398 10.2236 9.8122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31481_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31481_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31482_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31482_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:03.09 +48:45:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 1.462 390541857261634304 010.01324736511 +48.76489868347 10.1978 9.7480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31484_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31484_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:05.27 +45:27:01.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)
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Considering the candidate 31485_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31485_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:54:01.49 +50:35:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 1.208 415036502427305088 013.50600332428 +50.59239247377 10.2936 9.9193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31486_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31486_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:23.82 +48:24:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 2.030 390529526414760832 010.09853830898 +48.41077532435 10.1018 9.6605 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31489_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31489_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:47.38 +49:14:19.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)
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Considering the candidate 31490_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31490_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31491_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31491_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:51.51 +45:31:11.0 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 31493_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31493_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31496_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31496_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31497_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31497_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:14.59 +44:17:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 2.742 387818680493913344 009.31071113004 +44.28514843345 9.8728 9.4411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31498_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31498_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31500_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31500_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:21.80 +42:55:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 2.025 387598434571174656 009.84033395583 +42.93015570535 9.6832 9.3541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31502_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31502_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31503_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31503_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31504_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31504_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31505_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31505_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:42.71 +46:08:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 1.458 389115588819807744 008.42848494764 +46.14750946215 9.6758 9.2775 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 31506_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31506_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:19.09 +43:39:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 1.558 387714394391333120 009.08005842749 +43.65278188865 9.5876 9.2491 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 31507_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31507_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:50:30.03 +50:34:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 2.778 415000974457835008 012.62397192504 +50.57643754899 10.0846 9.7018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31508_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31508_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31510_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31510_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:50.14 +49:42:12.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)
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Considering the candidate 31511_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31511_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31512_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31512_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31514_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31514_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31516_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31516_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31520_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31520_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:22.61 +43:26:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)GAIADR2_OUTPUT=# 3.161 387641345587578624 009.84361704720 +43.43690494256 9.7204 9.3556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31521_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31521_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31522_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31522_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:50.88 +42:59:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 3.508 387423818380396416 010.46072417970 +42.99377462728 9.5785 9.1866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31523_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31523_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:12.04 +49:53:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.69, MAG_FAINT_SEARCH_LIMIT=11.67)GAIADR2_OUTPUT=# 3.719 414677138223228800 011.29875499725 +49.88562894583 9.6991 9.2647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31526_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31526_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31527_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31527_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31528_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31528_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31529_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31529_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31530_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31530_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:52.96 +43:27:47.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31532_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31532_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31533_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31533_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31534_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31534_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 31536_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31536_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31537_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31537_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:10.29 +44:50:14.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.31, MAG_FAINT_SEARCH_LIMIT=11.29)
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Considering the candidate 31538_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31538_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31539_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31539_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31540_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31540_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:42.12 +45:46:49.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31543_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31543_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 31544_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31544_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:02.16 +43:22:34.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31545_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31545_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31547_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31547_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:37.23 +43:38:13.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31550_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31550_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:40.02 +50:41:40.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31552_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31552_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31553_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31553_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:45.25 +42:31:33.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31554_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31554_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31555_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31555_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31556_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31556_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:10.91 +49:59:14.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31557_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31557_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:29.54 +47:54:55.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31558_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31558_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:41.47 +49:50:02.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31559_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31559_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:38.29 +50:35:12.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31560_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31560_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:02.32 +50:29:38.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31562_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31562_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:11.55 +49:23:27.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31563_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31563_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:25:03.36 +50:43:48.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31564_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31564_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:25:48.20 +49:39:32.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31565_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31565_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:38.27 +50:13:28.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31566_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31566_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:36.26 +50:06:59.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31567_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31567_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:17.04 +50:07:47.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31568_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31568_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:54.21 +45:00:14.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31569_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31569_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:04.39 +50:00:14.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31571_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31571_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:46.49 +50:15:34.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 31573_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31573_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31575_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31575_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31580_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31580_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31581_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31581_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31583_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31583_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31584_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31584_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:45.43 +50:01:22.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.52, MAG_FAINT_SEARCH_LIMIT=11.50)
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Considering the candidate 31585_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31585_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31586_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31586_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31587_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31587_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31588_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31588_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31589_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31589_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:38.59 +50:24:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.61, MAG_FAINT_SEARCH_LIMIT=11.59)GAIADR2_OUTPUT=# 5.175 391706965928784000 007.66298540288 +50.40727660935 9.4173 9.0957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31591_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31591_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:18.48 +50:29:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.68, MAG_FAINT_SEARCH_LIMIT=11.66)GAIADR2_OUTPUT=# 2.288 394678494883219456 006.57675961062 +50.48489476133 9.2073 8.4242 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 31592_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31592_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31593_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31593_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31595_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31595_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31596_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31596_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31597_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31597_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31598_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31598_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31599_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31599_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:11.50 +50:35:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)GAIADR2_OUTPUT=# 4.013 391759914285474176 007.29966358176 +50.59738682277 9.6577 9.3476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31600_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31600_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31602_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31602_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:43.94 +50:40:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 1.852 391739848198259712 007.68388235727 +50.67582619530 9.9122 9.8143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31603_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31603_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:25.58 +49:59:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)GAIADR2_OUTPUT=# 4.830 391691293589856512 007.85850924810 +49.98818341604 9.8375 9.3817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31604_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31604_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31606_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31606_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:16:04.65 +50:11:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 4.666 403335366543605248 019.01961309056 +50.19575946633 11.4710 9.2860 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31607_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31607_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31608_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31608_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31609_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31609_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:10.93 +50:45:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 5.309 394775771601571072 006.54378997895 +50.75272278238 9.7045 8.9763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31610_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31610_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:48.64 +50:07:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 4.391 391658621778932224 006.95456655251 +50.12126915919 9.9728 9.5844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31611_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31611_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:25:57.40 +50:25:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.26, MAG_FAINT_SEARCH_LIMIT=12.24)GAIADR2_OUTPUT=# 0.761 394676639457350144 006.48924353040 +50.42492792216 10.0002 9.7428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31612_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31612_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31614_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31614_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31615_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 31615_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 31616_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31616_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:41.94 +48:12:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 4.240 391055608368519936 006.92647161446 +48.20445978171 10.1910 9.8827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31617_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31617_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 31620_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31620_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:14:22.25 +47:04:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 1.447 401399500227686400 018.59293181641 +47.08028862023 11.5020 10.1868 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31623_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 31623_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:41:48.34 +46:35:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.970 351082206006878208 025.45137831972 +46.59687921636 12.1437 11.4654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 10177_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 10177_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 12996_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 12996_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 12234_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 12234_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 09136_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 09136_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 05978_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 05978_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 05521_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 05521_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 02708_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 02708_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 03524_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 03524_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 11631_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 11631_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 10497_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 10497_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:09:30.32 +47:14:31.3 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 96s
Prepared the HTML report for the field And-02-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 ####
00:45:56.25 +50:23:15.7
01:26:27.60 +49:53:58.1
00:58:20.83 +49:25:06.4
01:10:12.93 +49:10:15.4
01:14:04.52 +47:52:07.5
01:16:19.81 +47:27:31.0
01:33:35.62 +46:31:13.7
01:25:48.53 +46:24:13.0
01:15:42.26 +46:12:18.4
00:29:32.62 +49:25:24.8
00:44:52.14 +46:14:18.9
00:34:34.69 +42:09:25.3
00:54:37.50 +49:28:21.1
00:38:39.17 +43:48:36.1
00:33:45.23 +42:24:49.0
00:35:55.68 +42:23:43.1
00:40:58.52 +41:43:55.5
00:42:32.09 +40:57:18.8
00:39:19.95 +41:55:34.6
00:46:22.18 +50:04:38.5
00:52:57.44 +50:46:08.6
00:33:22.70 +49:51:24.6
00:34:27.80 +49:19:12.3
00:40:15.19 +50:49:23.2
00:42:38.80 +49:34:51.5
00:28:11.05 +50:28:08.9
00:33:55.33 +48:39:10.4
00:35:43.70 +41:45:08.4
00:28:05.04 +49:10:14.5
00:31:28.44 +49:04:22.2
00:36:27.59 +50:58:06.8
00:25:16.24 +50:31:57.6
00:46:51.43 +42:18:06.4
00:32:50.53 +49:19:44.5
00:26:49.68 +50:46:16.7
00:55:15.09 +49:39:22.0
00:36:48.66 +50:42:52.3
00:31:44.18 +50:02:56.2
01:31:58.34 +45:46:20.7
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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
SExtractor catalog cache: saved And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat to cache
SExtractor catalog cache: saved And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
Creating symlink local_wcs_cache/wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
Creating symlink local_wcs_cache/wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
Creating symlink local_wcs_cache/wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits exists and is non-empty
wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits exists and is non-empty
wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits exists and is non-empty
wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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 01:12:00.218 +45:59:53.67
Second-epoch image center 01:11:57.773 +46:00:02.51
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 01:12:00.218 +45:59:53.67
Second-epoch image center 01:12:01.103 +46:00:06.97
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 01:11:57.773 +46:00:02.51
Second-epoch second image center 01:12:01.103 +46:00:06.97
Angular distance between the image centers 0.00972 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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits &> /tmp/tmp.ourFYW9eEp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits &> /tmp/tmp.B0MPgztbtB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits &> /tmp/tmp.YoRAA6hoNs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits &> /tmp/tmp.3bvRrN2ZWP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
Calibrating the magnitude scale
Found non-empty wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits and wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits and wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat
Found non-empty wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits and wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat
The reference image (wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits) and catalog (wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat) found
'wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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 12072 out of 153071 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.801429
a=0.000000 b=1.000000 c=22.801429
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1223 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
2.0 pix And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
3.7 pix And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
3.7 pix And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
Limiting magnitude estimates:
15.5 mag. And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
15.5 mag. And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
14.4 mag. And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
14.5 mag. And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.7 (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.ourFYW9eEp (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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits' -> 'wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
Checking if the catalog wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits
WCS catalog name: wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=17331, passed=153037
Got 153037 stars (including 135496 good ones) from the SExtractor catalog wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat
util/solve_plate_with_UCAC5 got 153037 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 934 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits -region wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-02-Q2b1x1_2025-12-22_23-02-36_20.00sec_-14.90C_LIGHT_0212.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.B0MPgztbtB (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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits' -> 'wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
Checking if the catalog wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits
WCS catalog name: wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=42, blended=17215, passed=153176
Got 153176 stars (including 135718 good ones) from the SExtractor catalog wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat
util/solve_plate_with_UCAC5 got 153176 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 932 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: 0.42"
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 932 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: 0.44"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits -region wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-02-Q2b1x1_2025-12-22_23-03-16_20.00sec_-15.00C_LIGHT_0213.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.YoRAA6hoNs (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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
WCS_IMAGE_NAME=wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
WCS-calibrated image found: wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
Checking if the catalog wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits alredy exist and is non-empty...
Catalog wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits
WCS catalog name: wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=10022, passed=59291
Got 59291 stars (including 49223 good ones) from the SExtractor catalog wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat
util/solve_plate_with_UCAC5 got 59291 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (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 0.010420 (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 926 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: 0.94"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.99"
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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.99"
Estimated accuracy of the plate solution: 1.10"
Excluding outliers - 920 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits -region wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-02-Q2b1x1_2026-02-21_21-37-42_20.00sec_-15.00C_LIGHT_0082.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.3bvRrN2ZWP (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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
WCS_IMAGE_NAME=wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
WCS-calibrated image found: wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
Checking if the catalog wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits alredy exist and is non-empty...
Catalog wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat corresponding to the image wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits
WCS catalog name: wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=10085, passed=59485
Got 59485 stars (including 49352 good ones) from the SExtractor catalog wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat
util/solve_plate_with_UCAC5 got 59485 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 927 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: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.98"
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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.98"
Estimated accuracy of the plate solution: 1.06"
Excluding outliers - 922 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_And-02-Q2b1x1_214051_TTUQ2b1x1_21509_iasfEANj/And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits -region wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083.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-02-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
Adding exclusion_list_gaiadr2.txt__out132140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out138895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175773.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175828.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175839.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175937.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175956.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out175999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176343.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176498.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176564.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176565.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176625.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176647.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out176972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out175852.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out176376.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out176389.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out176415.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out176788.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out176875.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out04656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out106955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163782.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164137.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175710.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175776.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175780.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176230.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176242.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176272.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176350.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176422.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176519.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176587.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176610.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176646.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176789.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176864.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176993.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177046.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177050.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177098.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177281.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177382.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177453.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177525.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177555.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177559.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177631.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out70664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73227.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94276.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 895s
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: 292s
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Considering the candidate 175539_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175539_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:59:38.55 +49:08:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 3.697 356870280031382144 029.91017782786 +49.14956784798 13.4963 12.7451 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175540_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175540_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:55:12.25 +50:02:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 4.887 357739096079333632 028.79913220984 +50.04166565873 13.4815 12.9306 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175541_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175541_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:58:42.74 +49:17:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 3.287 357625610160481920 029.67908764971 +49.29069146856 13.4837 12.6364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175546_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175546_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:50:52.87 +45:46:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.564 350105534741147904 027.72048037103 +45.77013614591 14.3231 13.7126 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175554_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175554_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:55:41.17 +50:08:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.620 357741093240611072 028.92129303313 +50.13501827379 13.2151 12.5068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175560_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175560_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:21.96 +43:49:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.974 382503293391233664 007.84180432940 +43.81706405189 12.0377 11.4851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175574_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175574_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175579_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175579_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:48:58.54 +49:52:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.881 357866025249586048 027.24509721043 +49.87541511560 14.0861 13.7851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175580_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175580_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175582_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175582_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:50:29.18 +48:30:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.037 357179719538216192 027.62105717523 +48.51243494350 13.8583 13.5173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.037#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175585_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175585_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:36:26.50 +42:54:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.234 348755609340510336 024.11164164192 +42.91400973624 14.0724 13.6174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175588_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175588_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175592_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175592_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175593_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175593_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:01:28.44 +50:23:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 5.044 402789390301171456 015.36807509888 +50.38726347472 13.0648 12.3719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175597_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175597_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175600_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175600_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 175601_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175601_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:48:58.18 +44:49:52.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
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Considering the candidate 175605_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175605_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:48.50 +42:59:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.334 382369599649843072 007.45372608011 +42.99739675858 11.7889 11.2802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175610_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175610_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175616_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175616_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:26.41 +46:18:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.776 388425537896319744 009.35910181150 +46.31208290638 12.4895 12.0265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175617_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175617_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175619_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175619_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175620_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175620_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175621_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175621_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175622_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175622_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175623_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175623_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:07.78 +45:51:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.846 389058242416551424 008.53088466662 +45.85388635564 12.2485 11.7510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175624_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175624_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:57:59.63 +49:30:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.866 357654953377014016 029.49729889211 +49.50832149333 12.9200 12.2041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175625_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175625_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175627_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175627_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175628_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175628_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:46.52 +48:08:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.315 390347694678158976 011.94467361001 +48.14412071658 12.7479 12.2723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175629_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175629_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:06.25 +41:19:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 5.175 381230750418720256 009.77666424388 +41.33255373061 12.1877 11.7729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175630_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175630_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175631_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175631_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:24.46 +44:41:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 3.555 387854105384224128 009.35285678636 +44.68750452719 12.3979 11.9524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175637_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175637_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:12.44 +43:36:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.627 382448420889067392 008.30360684389 +43.60630571368 11.9105 11.4141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175638_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175638_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:51.93 +42:29:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 4.521 387362859908093824 010.96575568367 +42.49653083839 12.5048 11.9460 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 175639_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175639_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175640_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175640_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175643_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175643_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175644_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175644_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:25.21 +49:14:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.395 390660398359371264 010.35724214944 +49.24879448669 12.3417 11.8969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175646_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175646_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175647_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175647_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:49.83 +43:25:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.305 387506075594299520 011.20851954064 +43.42028759037 12.4526 11.9940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175649_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175649_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175650_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175650_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:40.61 +43:00:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.439 387427323073868928 010.67053953777 +43.00473877770 12.4909 12.0613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175651_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175651_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175653_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175653_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:30:44.33 +46:37:53.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 175655_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175655_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:54.41 +42:47:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 4.768 387596643569406336 009.72658793886 +42.79618247123 12.0883 11.6600 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175656_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175656_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:21.03 +43:37:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.952 387552426881182592 010.33866618703 +43.61837810676 12.1809 11.6989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175658_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175658_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175659_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175659_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175661_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175661_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:25.67 +41:01:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.205 369216004607192960 011.60631530492 +41.03278484039 12.2518 11.7380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175662_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175662_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175664_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175664_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175665_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175665_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175666_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175666_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:58.34 +43:00:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.433 387602935696896512 009.99402115314 +43.01443937369 12.9371 12.3167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175669_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175669_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175671_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175671_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:36.07 +43:20:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.492 387504147153240192 011.15090109410 +43.34783517146 12.3614 11.7050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175674_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175674_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175675_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175675_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:25:17.92 +47:28:15.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 175676_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175676_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:55.19 +42:34:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 5.398 387393577514189824 010.48054224186 +42.57568644433 12.2565 11.7111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175677_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175677_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175679_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175679_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:33.15 +41:17:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 5.793 369278264453145600 011.13959014166 +41.29625701376 12.1702 11.7747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175681_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175681_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175682_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175682_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175684_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175684_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:57.61 +42:14:03.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 175685_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175685_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175686_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175686_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175687_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175687_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:34.18 +48:58:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.767 391345325383616896 008.39462206949 +48.97806391297 11.9914 11.2688 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175688_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175688_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175691_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175691_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175692_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175692_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:42.03 +43:14:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.788 387668283622473984 009.17573708773 +43.24533632319 12.1490 11.5303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175693_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175693_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175699_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175699_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175702_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175702_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:20.46 +42:12:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.218 387321284624686336 011.33494355223 +42.21080909425 12.4009 11.9755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175706_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175706_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 175709_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175709_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:28.78 +42:54:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.390 387378257367497728 010.87070868708 +42.90082504516 12.2195 11.8097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175710_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175710_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175711_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175711_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175713_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175713_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:41.58 +44:51:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.510 388233574335058048 009.67376765402 +44.85534775573 12.3485 11.9259 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175716_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175716_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175717_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175717_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:22.11 +43:43:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 4.581 387714978506881920 009.09369532615 +43.72222981168 12.1100 11.6182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175719_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175719_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175723_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175723_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:58.78 +50:16:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.677 414828729090190464 010.74660724894 +50.27261028247 12.0158 11.4445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175726_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175726_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175728_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175728_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175729_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175729_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:10.76 +42:53:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 4.869 387600526219846016 010.04414744013 +42.89956128637 12.3744 11.8301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175730_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175730_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175733_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175733_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175734_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175734_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:47.70 +42:31:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.840 375346232905721856 011.44843916771 +42.52642902802 12.2519 11.8416 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 175735_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175735_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:54.96 +41:55:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.921 375313930455533056 011.97783995398 +41.93361547595 12.9122 12.3890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175736_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175736_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:11.68 +41:36:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.662 381298709684828928 010.79786261090 +41.60545926082 12.0824 11.6571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175737_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175737_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:13.26 +43:22:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 5.700 387672097553422592 009.30538656474 +43.37369128239 12.0927 11.5877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175738_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175738_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:43.96 +42:02:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.567 381464151824908928 009.43398782933 +42.04472538431 11.9675 11.4573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175739_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175739_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:16.37 +47:01:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 3.147 390148202037473792 011.81944500781 +47.02762977073 12.8172 12.3295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175740_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175740_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:48.90 +43:57:50.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 175741_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175741_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175742_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175742_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:06.03 +42:58:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 5.321 387428796259220352 010.52622567922 +42.98298940456 12.2959 11.9290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175743_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175743_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175745_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175745_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:52:13.61 +41:33:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.488 375138317832748800 013.05742273934 +41.56182066318 12.6141 12.1798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175748_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175748_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:15.60 +46:04:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.400 389067416466636416 008.56648575856 +46.07621249322 11.9938 11.5404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175749_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175749_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:43.87 +41:43:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 5.504 381479304468385152 008.93450039902 +41.72978777892 11.7019 11.0997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175752_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175752_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175754_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175754_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175755_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175755_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175757_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175757_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:28.21 +43:35:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 5.812 382448111651422848 008.36916283605 +43.58425304236 11.5854 11.2554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175759_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175759_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175761_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175761_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:26.08 +44:34:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.092 387849153285883776 009.61006367536 +44.58392180333 12.0982 11.6842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175763_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175763_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175765_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175765_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175767_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175767_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175768_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175768_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:29.86 +50:18:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 3.305 414969814474560384 012.37342815872 +50.30008374015 12.2027 11.7806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175771_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175771_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175773_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175773_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:54.64 +43:29:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 5.025 387873896593695360 011.47899740757 +43.49175808301 12.5341 11.7597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175775_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175775_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175776_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175776_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175779_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175779_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:25.58 +44:22:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.953 387840082314967552 009.60725159235 +44.36741695173 11.9819 11.5591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175780_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175780_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175781_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175781_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175782_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175782_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:26.45 +50:14:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.684 414825572293286400 010.86093088190 +50.23919073443 12.2165 11.8528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175783_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175783_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:39.56 +45:34:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 4.104 388886924761405696 007.16643496903 +45.57617884155 11.5018 11.0465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175788_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175788_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175790_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175790_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:53.37 +42:06:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 3.390 382262057964720512 007.97148303986 +42.10291983613 11.5095 11.0378 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175791_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175791_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175792_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175792_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:54:28.23 +50:42:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.688 415043756632772736 013.61773207769 +50.71009544493 12.5813 12.1725 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175793_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175793_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175794_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175794_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:16.22 +41:03:23.5 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 175795_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175795_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175796_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175796_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175797_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175797_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175800_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175800_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:46.20 +42:05:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.592 375354612384831872 012.44202422215 +42.08557180913 12.1832 11.5525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175803_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175803_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175805_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175805_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:55:38.70 +51:01:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.183 403068077841290112 013.91072756561 +51.01916341001 12.2050 11.6802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175806_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175806_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175808_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175808_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:52:23.03 +49:29:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 3.069 414510660992079232 013.09708651121 +49.49126893375 12.6646 12.2545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175809_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175809_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175811_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175811_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:46.23 +42:01:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.081 381509510974740352 008.94377661937 +42.02038242504 11.5396 10.8070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175812_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175812_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175813_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175813_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:44.25 +42:44:56.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 175815_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175815_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175816_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175816_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:19.27 +49:22:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 4.170 391412807910611712 009.33204391487 +49.37183829336 11.8929 11.4354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175817_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175817_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:54:44.83 +50:54:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.102 415070243691396992 013.68673212697 +50.91213967811 12.2784 11.9574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175819_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175819_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175822_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175822_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:30.49 +50:35:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.793 414852338529066112 010.62812083539 +50.59544948476 11.9823 11.4831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175825_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175825_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175827_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175827_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175828_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175828_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:58.80 +43:58:36.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 175829_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175829_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:38.35 +43:42:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 5.034 387706285493075328 009.41011909594 +43.70632265827 11.9290 11.4580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175830_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175830_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:01.98 +42:48:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.251 387409932751229184 010.25786529688 +42.80403020228 12.0155 11.4729 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 175831_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175831_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:56.23 +41:56:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 5.278 381345237072678784 010.23562823548 +41.94132754929 11.8247 11.1624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175832_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175832_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175833_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175833_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:48:31.84 +50:08:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.272 414604153839445376 012.13301373889 +50.14280218716 12.0421 11.6140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175835_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175835_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:36.25 +45:26:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.990 389011405796789632 008.90086468715 +45.44896133516 11.9641 11.7180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175836_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175836_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175838_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175838_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:36.37 +40:57:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.794 381024901224742912 008.90288439537 +40.96025222260 11.5308 10.7583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175839_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175839_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:22.92 +48:32:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 0.749 390391911363383168 011.59566582352 +48.53784337095 12.2115 11.7602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175841_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175841_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:54.02 +47:38:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.119 390052574587270400 010.47636579997 +47.63936993177 12.2053 11.8067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175842_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175842_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:07.10 +42:57:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.254 387463813116198016 011.27953905395 +42.95843086495 12.2272 11.7566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175843_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175843_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:22.65 +47:26:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.438 390749527521990144 009.09439824608 +47.44354533974 12.1495 11.9063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175844_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175844_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:09.04 +42:08:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.897 375331213403921920 011.53795571596 +42.14428696817 12.1732 11.7045 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 175846_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175846_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175848_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175848_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:52.87 +42:49:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.135 387455738577698560 011.22035062373 +42.82949177264 12.2008 11.6437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175849_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175849_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:35.03 +41:28:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.246 381293452643534464 010.89614774698 +41.47011540080 11.8969 11.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175850_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175850_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:12.13 +49:48:54.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 175851_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175851_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175852_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175852_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:19.10 +42:26:47.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 175854_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175854_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175855_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175855_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:50:10.14 +49:47:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.025 414531246773506944 012.54255095850 +49.79201392999 12.2648 11.7616 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 175857_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175857_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:28.98 +44:50:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 4.514 387870421963924224 009.12140970625 +44.83683008173 11.9551 11.5698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175858_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175858_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:22.10 +47:37:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.433 390107107790851584 009.84382858556 +47.61783627432 12.0205 11.5907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175860_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175860_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:22.66 +42:37:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.115 375431784357866880 011.84429085666 +42.62048211743 12.0075 11.6045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175862_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175862_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175863_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175863_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175864_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175864_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:57.19 +45:38:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.120 389072879662646144 008.23910791235 +45.64813239937 11.7163 11.2730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175865_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175865_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175867_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175867_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175868_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175868_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175869_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175869_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:43.63 +43:17:09.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 175871_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175871_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:33.77 +47:31:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.975 390786159300567552 008.14151853722 +47.52879131037 11.9983 11.5717 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 175872_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175872_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:31.22 +46:46:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.895 389953760277966976 009.87933213776 +46.77792374804 12.0541 11.6187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175873_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175873_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:35.03 +43:05:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.507 375477104852748928 011.64630972240 +43.08388640264 12.3451 11.9389 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 175874_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175874_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:50:38.62 +41:17:29.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 175876_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175876_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175879_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175879_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:36.52 +42:02:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.665 381544725410767488 009.65233724014 +42.04290068532 11.7252 11.0441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175882_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175882_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:40.63 +43:57:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.249 387749166447260416 009.91957468385 +43.95560714291 12.0770 11.6666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175883_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175883_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175884_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175884_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175885_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175885_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175886_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175886_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:34.33 +47:27:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.848 390070789547494528 009.89328835922 +47.46227343329 12.0643 11.5623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175887_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175887_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175888_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175888_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:32.14 +42:38:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.943 387450584616961792 011.38378345623 +42.64925296554 11.9371 11.5616 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 175889_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175889_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175890_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175890_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175891_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175891_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:09.26 +44:07:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.956 387810429860096768 009.28809047334 +44.12071942876 11.8797 11.4306 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 175892_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175892_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:50.86 +50:13:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.387 391701296572287232 007.96004132759 +50.22626895391 11.2767 10.5962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175894_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175894_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175896_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175896_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:05.02 +41:55:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.183 381881661301218944 007.76937199318 +41.92047577788 11.4777 11.0292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175897_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175897_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 175898_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175898_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:56.05 +44:45:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 2.966 388193815821585664 010.23412164975 +44.75471358784 12.1757 11.7332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175899_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175899_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175900_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175900_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:05.44 +50:43:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.872 414868002271153920 011.02260940897 +50.71803695739 11.8749 11.4062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175901_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175901_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:22.44 +42:18:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 4.324 387380765628358272 010.59424663666 +42.30295550924 11.9463 11.4762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175902_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175902_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:24.91 +45:10:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.591 388640801657297536 008.60329054748 +45.18137266803 11.7842 11.3446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175903_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175903_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:49.26 +47:09:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.377 390759801082121088 008.45735960436 +47.15191572269 11.7517 11.3545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175905_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175905_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175907_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175907_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:39.98 +43:25:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.301 387640417874643072 009.91691065030 +43.43225993015 11.8305 11.1412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175908_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175908_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175909_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175909_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175910_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175910_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:41.54 +45:48:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.136 389089612857502976 007.92427048080 +45.81232802369 11.3837 10.9532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175911_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175911_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:16.49 +45:39:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.144 389076521794891648 008.06888603351 +45.66138559453 11.6422 11.2826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175912_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175912_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:14:25.22 +44:47:48.9 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 175913_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175913_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:52.43 +46:47:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 5.872 389952111010526592 009.97045282047 +46.78586387604 12.1546 11.4894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175914_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175914_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175915_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175915_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175917_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175917_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175918_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175918_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175919_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175919_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175920_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175920_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175921_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175921_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175922_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175922_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:35.04 +43:47:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.414 387570427088134528 010.64716100760 +43.79241607718 12.2140 11.7878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175923_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175923_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175928_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175928_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:32.07 +49:31:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.460 414645114946917760 010.88384579321 +49.52427935087 12.0061 11.4950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175929_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175929_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:10.29 +44:51:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 4.441 388228587876794624 009.54390546418 +44.86288287165 11.7182 11.4719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175930_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175930_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175931_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175931_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:14.89 +46:48:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.855 389943417996559872 009.56133191675 +46.81218231085 11.9175 11.4404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175932_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175932_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:36.83 +42:11:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 4.103 381551017539222912 009.90418677786 +42.19828171672 11.5987 10.9064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175934_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175934_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175937_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175937_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:11.66 +43:15:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 4.242 387667802586136192 009.05017387973 +43.25640961286 11.7927 11.3412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175938_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175938_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:53.00 +41:36:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.348 381331832474985344 010.22043745559 +41.61193732769 11.7191 11.2560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175939_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175939_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:56.83 +50:03:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.574 414729124506961152 010.73747256854 +50.06330840717 11.9520 11.5277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175941_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175941_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175943_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175943_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:57.37 +48:00:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.198 390494376402511488 009.98857047975 +48.01078232204 11.8725 11.3658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175946_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175946_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:42.67 +49:30:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.026 414688610076367232 010.42746801649 +49.50264455872 11.8241 11.3083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175947_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175947_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175948_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175948_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175949_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175949_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175951_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175951_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175952_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175952_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175953_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175953_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175954_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175954_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:14.51 +42:20:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.224 387340461655385856 010.81006020844 +42.34351540499 11.9755 11.4767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175955_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175955_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175956_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175956_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:26.08 +40:52:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 5.490 381009263247880960 008.36036426514 +40.88176820001 11.2504 10.5970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175958_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175958_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:10.06 +41:22:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.836 375030153375389824 012.29226110888 +41.37676278649 12.0466 11.4838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175960_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175960_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175961_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175961_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:45.80 +45:19:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.789 388704027871122432 007.69202659104 +45.31785660376 11.0237 10.4938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175963_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175963_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:11.13 +45:53:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.504 388393686418872448 009.54645107068 +45.89784248403 12.2362 11.8024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.504#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175964_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175964_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:48:59.92 +41:52:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 4.207 375268197642803072 012.24932682754 +41.87994630757 12.1307 11.6433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175967_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175967_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:09.73 +44:59:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.572 388634788703049216 008.29135323686 +44.98788021528 11.6707 11.2413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175968_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175968_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175969_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175969_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:52.21 +46:40:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 4.985 389226257239893248 008.21954467072 +46.68157985232 11.5636 11.1357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175971_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175971_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:14.69 +41:24:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.707 381270504641893504 010.81119939948 +41.41639071636 11.8097 11.3625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175972_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175972_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:29.31 +46:38:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.846 389199667100527872 008.62388748277 +46.64956241515 11.7450 11.2879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175973_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175973_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175975_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175975_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175976_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175976_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:54.94 +48:53:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.238 390627589107815168 010.47997819442 +48.89396038240 12.0982 11.8409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175977_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175977_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:03.39 +48:36:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 3.739 390527224312442624 010.26569537942 +48.60237871699 11.7888 11.4499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175978_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175978_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:41.07 +46:46:45.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 175979_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175979_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175980_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175980_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:52.32 +47:27:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.070 390750145995630336 008.96840044808 +47.45912727180 11.5861 11.3539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175981_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175981_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:52.09 +44:09:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.043 387812766322304640 009.46801455179 +44.15421329276 11.7991 11.3362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175982_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175982_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 175983_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175983_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:26.76 +44:59:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.988 388634277604543360 008.36119884371 +44.99126821075 11.6319 11.1396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175984_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175984_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:26.36 +47:19:21.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 175985_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175985_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:55.16 +46:06:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 0.747 389068138018962560 008.48012749129 +46.10037125043 11.7555 11.1959 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 175986_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175986_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:04.66 +41:23:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 5.159 381280327224806528 010.27020487235 +41.39574982315 11.6786 11.0907 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 175987_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175987_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:21.61 +50:58:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.493 415637389831659904 010.09111715138 +50.97728431250 11.8111 11.3697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175988_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175988_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175990_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175990_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175991_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175991_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175992_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175992_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:34.75 +50:44:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 5.483 415580657604962560 008.89696662323 +50.74737504466 11.4433 10.9539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 175994_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 175994_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 175997_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175997_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:07.40 +44:53:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 4.913 388759411474047232 007.28245473172 +44.88923664162 11.3536 10.9061 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 175999_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 175999_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:13.00 +47:30:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.750 390751455965407744 009.05358490713 +47.50875844603 11.8761 11.3456 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 176000_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176000_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:50:38.62 +50:13:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 3.296 414919919835049088 012.65953938622 +50.22805708183 12.0288 11.6315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176002_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176002_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176005_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176005_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176007_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176007_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176008_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176008_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:40.29 +41:52:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.661 375301324728021760 011.41768161343 +41.87370118416 12.0733 11.6926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176009_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176009_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176010_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176010_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:00.83 +45:20:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.342 388268037152527616 009.50324533779 +45.34668648973 11.7822 11.3361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176011_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176011_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 176012_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176012_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:54:00.74 +50:04:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.329 402919613709481216 013.50405757011 +50.07580495422 12.3217 11.8748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176013_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176013_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:08.22 +45:13:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 3.529 388863079103066880 007.28554551548 +45.22261439389 11.3908 11.0921 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 176014_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176014_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (25.7") between the two second-epoch detections
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Considering the candidate 176015_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176015_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176016_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176016_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176017_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176017_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:00:26.59 +45:32:45.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
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Considering the candidate 176019_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176019_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:58.21 +50:19:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 2.026 415498267250163584 009.74191960568 +50.32557335725 11.8552 11.3424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176020_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176020_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176021_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176021_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176022_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176022_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176023_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176023_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:57.53 +44:30:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.795 387941615341901440 011.24167483649 +44.51234608517 12.1851 11.7507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176024_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176024_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:41.69 +43:05:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.208 387617877887706368 009.67331074207 +43.08416809928 11.9013 11.4785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176026_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176026_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176029_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176029_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:49.44 +48:17:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.719 390372468049471744 011.95511730034 +48.28919686646 12.3016 11.9309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176030_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176030_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:28.25 +47:07:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.357 390014611375420928 010.36899222197 +47.12824282886 11.9504 11.5202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176031_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176031_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176032_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176032_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176034_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176034_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176035_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176035_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176036_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176036_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176037_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176037_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176038_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176038_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176039_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176039_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:02.85 +41:34:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.482 381330801682834688 010.26213229063 +41.57797573619 11.5804 10.9817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176040_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176040_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176043_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176043_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:28.45 +42:35:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.088 387388668368126720 010.36897805284 +42.58698290937 11.7370 11.3208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176044_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176044_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:00.66 +44:02:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.859 387775868260165376 010.25331576046 +44.05023494492 11.9514 11.5762 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176045_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176045_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176046_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176046_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:51:50.29 +50:25:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.734 414948820674687104 012.95878556824 +50.42896755524 11.9873 11.5273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176047_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176047_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:58.04 +46:00:14.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)
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Considering the candidate 176048_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176048_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:45.76 +45:47:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.750 388388498098389888 009.19125845368 +45.78817367015 11.8048 11.3895 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 176049_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176049_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:01:36.33 +41:55:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 5.551 374785585054415232 015.40263022192 +41.92733805078 13.1315 12.4813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176050_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176050_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176051_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176051_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:54.98 +46:26:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.442 389182040554819712 008.97952245481 +46.44340439084 11.6179 11.2294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176052_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176052_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:57:00.72 +51:05:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.837 404555854513212800 014.25257313029 +51.09590762610 12.0683 11.6651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176053_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176053_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:34.51 +49:11:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.364 390659921621514240 010.39388884556 +49.19764336828 11.7445 11.4619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176054_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176054_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:13.40 +46:18:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 5.384 389305151496781312 007.05758829507 +46.30917980738 11.3391 10.8014 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 176055_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176055_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176056_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176056_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:52:17.06 +50:19:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 5.083 414946995308877824 013.07329039921 +50.32243684606 11.9556 11.5020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176057_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176057_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:35.56 +44:38:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 1.000 387859048890531200 009.14848633932 +44.63660409778 11.6244 11.1899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176058_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176058_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176060_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176060_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176061_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176061_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:44.50 +48:44:28.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)
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Considering the candidate 176064_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176064_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176065_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176065_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176066_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176066_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176067_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176067_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:30.08 +43:09:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.837 387630938883652352 009.87635457918 +43.15639611574 11.6131 11.2954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176068_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176068_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:41.16 +46:37:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.947 389224749709356544 008.17313858523 +46.63043322092 11.3924 10.9337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176069_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176069_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176071_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176071_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176073_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176073_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:26.93 +43:48:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.490 387578707785080704 010.36355120851 +43.80889023974 11.8920 11.4704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176076_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176076_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:57.90 +50:03:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.257 414773551649515136 011.24216930451 +50.05601896502 11.7252 11.2182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176077_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176077_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:05:50.51 +48:28:40.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)
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Considering the candidate 176079_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176079_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176080_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176080_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176081_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176081_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:08.92 +47:29:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 4.297 390832441868781056 009.28578706137 +47.48625447904 11.7720 11.3557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176083_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176083_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176084_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176084_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:11.68 +46:45:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.685 389247598935523840 008.54884418642 +46.76004809673 11.5647 11.1093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176085_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176085_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:20.16 +44:57:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.594 388212271297257088 009.83534876012 +44.95337619057 11.8981 11.4263 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176086_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176086_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176087_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176087_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176088_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176088_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:36.89 +47:18:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 0.879 390730870184058368 009.15402787322 +47.31477909408 11.6157 11.1429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176089_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176089_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:20.74 +46:02:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.878 389145580573575296 008.83796837189 +46.04331204681 11.6315 11.1664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176090_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176090_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:04.80 +41:43:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 5.224 381491025435406080 008.51927969441 +41.72945782087 11.3670 10.9104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176091_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176091_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176092_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176092_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:15:50.93 +50:17:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 5.727 403348006629278976 018.96129828592 +50.29265797016 12.5706 11.7812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176093_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176093_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:20.44 +46:33:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.537 389188186650669696 009.08367682502 +46.55262290109 11.6163 11.1456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176094_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176094_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:36.51 +42:42:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.177 387451168732511616 011.40256614333 +42.70973617302 11.8149 11.3373 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 176095_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176095_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176096_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176096_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:57.33 +50:48:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.847 415616464747350784 009.74096049320 +50.81533444850 11.4824 11.0054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176097_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176097_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176100_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176100_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176101_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176101_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:05.49 +49:36:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.062 414552515451632768 012.27170552343 +49.60149729677 11.9802 11.5143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176104_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176104_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:35.74 +41:47:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 5.228 381315481539313792 010.64721796284 +41.78409515725 11.2196 10.8718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176105_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176105_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176106_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176106_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176108_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176108_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176109_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176109_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176111_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176111_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:05.84 +41:58:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.765 381451202498750848 009.52484698276 +41.97780345774 11.4137 10.9406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176112_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176112_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:52:17.83 +49:45:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.625 414522789979707008 013.07483568295 +49.75328318257 12.1008 11.6545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176113_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176113_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176115_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176115_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:41.97 +44:44:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 3.468 388229107569081728 009.42622903772 +44.74944392074 11.6356 11.1984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176117_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176117_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:09.17 +47:49:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.242 390843883661536896 009.28992907513 +47.82795367496 11.5800 11.1246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176118_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176118_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176119_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176119_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:12:28.67 +47:26:51.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 176121_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176121_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176124_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176124_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176125_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176125_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176127_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176127_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176129_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176129_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176131_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176131_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176132_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176132_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176134_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176134_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176135_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176135_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176137_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176137_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:26.48 +41:18:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.428 381230093289608704 009.85915609841 +41.30051924613 11.3949 10.9874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176138_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176138_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176139_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176139_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:33.72 +44:00:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 2.788 387587572597573504 010.39121919947 +44.01179844238 11.8568 11.3750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176140_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176140_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:33.14 +49:30:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 4.062 390683595481148160 010.13978083963 +49.50718541723 11.3279 10.7952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176142_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176142_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:56.10 +47:37:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.322 390412325347632000 010.73381268042 +47.62914256364 11.9033 11.4254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176144_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176144_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:05.54 +42:24:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 4.587 381614961012115072 009.02271984686 +42.40407894870 11.3359 10.6878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176147_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176147_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176148_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176148_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176152_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176152_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:29.56 +50:15:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.217 414784611186126208 011.12368405073 +50.26640337849 11.7041 11.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176153_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176153_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:14.32 +49:00:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.499 390606767106545280 010.81029151458 +49.01237025650 11.8131 11.3462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176154_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176154_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:52:06.27 +49:37:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 2.428 414514646721724032 013.02677725546 +49.62336306768 11.9529 11.5580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176155_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176155_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:06.14 +49:52:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.031 414679062368268800 011.02583410003 +49.86770709504 11.5545 10.9087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176156_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176156_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:48:08.13 +41:13:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 5.052 375209992246002560 012.03567546845 +41.23034128424 11.6903 11.3160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176157_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176157_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176159_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176159_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:24.36 +42:53:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 3.680 387598297132138880 009.85012688902 +42.89304082485 11.5722 11.1687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176160_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176160_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:05.25 +43:13:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 1.798 387622795625553408 009.52215685729 +43.22712189251 11.5817 11.0962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176161_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176161_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:02.02 +43:34:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 5.467 382494188060574976 007.76003673860 +43.57195317319 11.2588 10.7919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176162_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176162_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:21.69 +50:47:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.690 415194660304697088 011.34048651952 +50.78577251577 11.6877 11.1054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176163_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176163_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176164_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176164_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:09.66 +46:03:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 5.493 388418704605425792 009.54113476097 +46.06125799669 11.6019 11.2096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176165_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176165_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176169_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176169_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:39.30 +45:06:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.220 388241232259741056 009.41330250179 +45.10853959965 11.6833 11.1087 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 176171_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176171_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:56.27 +45:17:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.552 388267659195416192 009.48273502213 +45.29852933422 11.6576 11.1471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176172_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176172_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:14.28 +45:51:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 1.961 389048965287202432 008.81006887637 +45.86495726142 11.5238 11.1320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176173_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176173_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:44.64 +43:58:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.967 387727794689281280 008.93731569800 +43.96657556648 11.5826 11.1767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176176_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176176_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:44.44 +41:09:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 5.706 375012045793411456 012.43546271717 +41.15406915328 11.8870 11.4863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176181_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176181_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176183_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176183_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176185_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176185_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:28.76 +44:09:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 176186_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176186_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176187_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176187_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:25.36 +49:06:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.291 391396010297080832 009.60609331447 +49.10946971730 11.4861 11.0467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176190_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176190_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:39.87 +44:27:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 0.384 388583219033421056 008.66603190366 +44.45041684408 11.8922 11.4712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.384#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176193_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176193_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176195_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176195_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176197_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176197_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:05.19 +49:06:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 5.574 390648342389694592 010.01931593267 +49.11155282496 11.6302 11.2118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176198_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176198_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176199_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176199_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176200_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176200_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:38.41 +50:41:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.048 415180955067461504 011.66042103276 +50.68864524047 11.6651 11.3665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176201_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176201_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:23.15 +42:04:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.820 381545618763964032 009.59672706664 +42.07706306032 11.5253 10.9193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176202_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176202_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176203_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176203_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176204_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176204_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:38.84 +43:55:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.276 387580838088856192 010.41057016512 +43.91747812264 11.6848 11.2288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176206_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176206_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:01.18 +47:45:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 5.144 390103637457223936 010.00700306252 +47.75506079084 11.6910 11.2098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176207_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176207_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176208_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176208_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:06.81 +41:35:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.125 381254286839685760 009.77778544594 +41.59066319225 11.4183 10.9904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176211_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176211_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176212_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176212_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:23.01 +42:39:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.985 375441684258217344 011.59593727227 +42.66496424177 11.6781 11.2564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.985#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176214_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176214_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:50:21.42 +41:28:09.7 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 176215_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176215_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:38.71 +49:29:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 5.541 391428995645995392 009.90956568660 +49.49238976325 11.5248 11.0292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176216_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176216_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:36.43 +50:01:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.351 414587871622196352 012.40180885474 +50.03354167607 11.7516 11.2782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176217_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176217_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176218_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176218_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:46.78 +47:57:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.542 390859757860610432 008.94485941971 +47.95518463387 11.4659 10.9553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176219_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176219_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:23.96 +45:35:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.007 388370390516289536 009.60052814998 +45.58893933819 11.3713 11.0050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176220_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176220_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176221_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176221_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176222_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176222_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:27.96 +47:35:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 2.463 390224996052552320 011.36751053175 +47.58341889554 11.7291 11.5561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176224_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176224_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:56.06 +43:45:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.625 387743329587890816 010.23436494392 +43.75994508985 11.6511 11.2198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176226_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176226_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176227_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176227_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176228_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176228_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:12.61 +45:38:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.749 389042780534466176 009.05283143308 +45.64219722610 11.5439 11.0826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176229_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176229_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:09.15 +46:46:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 3.216 390690329990962048 009.28827198386 +46.77585992639 11.6525 11.2569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176230_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176230_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176231_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176231_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176232_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176232_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 176233_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176233_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:19.68 +44:29:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.192 388032290691346304 011.33320189148 +44.49126027677 11.8430 11.6322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176235_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176235_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:12:03.64 +45:23:40.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)
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Considering the candidate 176236_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176236_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176237_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176237_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:40.58 +48:49:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 4.366 390967991035996032 008.17085702123 +48.82472840110 11.3048 10.8440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176239_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176239_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:08:53.12 +45:08:11.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)
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Considering the candidate 176240_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176240_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176241_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176241_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:08.73 +42:26:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 5.736 387397601900137344 010.28820363630 +42.44181950841 11.4167 10.8965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176242_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176242_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176245_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176245_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:52.52 +50:50:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.724 415195867193512576 011.46920953168 +50.84713803170 11.5577 11.1495 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 176246_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176246_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:44.65 +43:50:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.164 387746726905172480 009.93609610485 +43.84657214821 11.7762 11.3063 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176247_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176247_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:16.84 +44:42:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.487 388179148509508224 009.82230125054 +44.70665852672 11.5500 11.1496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176248_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176248_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:00.09 +49:48:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.675 414754821295585536 011.50077388630 +49.80144694843 11.6722 11.3756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176249_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176249_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:58.89 +44:17:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.767 387978586420392448 010.99561591689 +44.29826516201 11.6953 11.2743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176250_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176250_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:53:34.83 +50:52:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 3.054 415049700867449088 013.39428164202 +50.88118849581 11.7192 11.3732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176251_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176251_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176252_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176252_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176254_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176254_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176255_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176255_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:36.29 +41:35:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.152 375279845594127360 011.65043986148 +41.58339179351 11.6486 11.1874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176257_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176257_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176258_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176258_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176260_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176260_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:29.40 +44:45:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 4.194 388613936639587200 008.87132012928 +44.75342055531 11.2746 10.8656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176261_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176261_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:21.50 +48:26:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 3.405 390475272388075520 010.58818385532 +48.43481860021 11.6978 11.2615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176262_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176262_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176264_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176264_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:05.98 +48:55:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 4.103 391306503178706048 009.27658851590 +48.91658618150 11.3225 10.8468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176265_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176265_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176266_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176266_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176267_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176267_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:17.87 +48:46:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 4.343 391303101564662528 009.32607694627 +48.77123005190 11.3931 10.9851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176269_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176269_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176270_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176270_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176271_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176271_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:36.94 +43:24:59.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
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Considering the candidate 176272_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176272_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176274_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176274_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 176275_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176275_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:48:07.12 +49:05:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.840 414441597919601664 012.02909595254 +49.08745953380 11.8073 11.3034 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 176276_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176276_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:57.38 +48:39:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 5.879 391266611522553600 009.49154965958 +48.65633191952 11.4731 11.1352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176277_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176277_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 176278_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176278_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176279_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176279_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176280_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176280_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176281_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176281_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176282_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176282_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:54:47.60 +50:43:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 5.113 403034512674722432 013.69666337349 +50.71783724219 11.4799 11.1036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176284_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176284_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:05.57 +41:50:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 5.824 381445803724626304 009.77105578870 +41.83559310948 11.1454 10.6318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176286_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176286_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:51.93 +43:06:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 3.830 382399874875669504 008.46709883014 +43.11240997151 11.1578 10.5450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176288_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176288_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:18.49 +42:22:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.200 387382513678448256 010.57663178760 +42.37505301976 11.4107 10.9895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176289_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176289_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:46.47 +46:56:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 1.360 389913181426928768 010.19347986352 +46.94925333162 11.5141 11.2881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176290_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176290_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:31.89 +48:03:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 4.506 390881713733399936 009.13424020961 +48.05908782573 11.3715 10.9498 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 176291_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176291_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:59.57 +48:04:07.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)
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Considering the candidate 176292_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176292_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176293_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176293_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176294_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176294_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176295_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176295_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:14.06 +41:16:48.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)
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Considering the candidate 176298_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176298_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176299_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176299_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176300_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176300_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (30.8") between the two second-epoch detections
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Considering the candidate 176302_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176302_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176303_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176303_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176305_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176305_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176307_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176307_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176308_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176308_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:48:27.88 +50:52:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 5.843 415022556672751744 012.11363359631 +50.87222501185 11.5826 11.0699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176309_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176309_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:25.45 +47:25:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 5.049 390829177693647104 009.35439896236 +47.42852218437 11.2890 10.8209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176310_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176310_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:51.44 +47:47:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 5.895 391004103121157760 007.96657235865 +47.79043620113 11.1676 10.7322 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176311_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176311_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:35.25 +41:36:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 4.240 381290124052426240 010.39738780958 +41.61694688367 11.3446 10.9417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176312_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176312_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:44.60 +41:28:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.619 375230195772190720 011.68525439298 +41.47436023494 11.4902 11.1044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176314_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176314_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:29.07 +49:55:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.816 414725065758749056 010.62046221359 +49.92878662538 11.4319 11.0663 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 176315_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176315_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:15.05 +47:24:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.506 390034467006486656 010.81212232826 +47.40275549841 11.5715 11.2170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176316_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176316_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:46.94 +46:06:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.136 389150189077443840 009.19680973190 +46.10750463338 11.3965 10.9367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176317_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176317_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:27.39 +41:12:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 2.482 369219651038361856 011.61446005350 +41.20261384542 11.4710 11.0608 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 176318_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176318_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176319_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176319_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:50.29 +41:24:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 4.209 369283216553938816 010.95919066970 +41.40322189891 11.3617 10.9901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176320_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176320_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176322_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176322_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:09.72 +47:16:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 3.536 390732764267789696 009.28907201103 +47.27861641128 11.3291 10.9707 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 176323_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176323_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176324_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176324_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:59.48 +45:57:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.506 388394201814942848 009.49801558159 +45.96667215494 11.3249 11.0374 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 176325_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176325_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:18.67 +42:29:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 4.039 387389935381928192 010.57681181934 +42.49191381278 11.4095 10.9266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176326_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176326_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:54:39.82 +50:49:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.713 415046088794323712 013.66689250750 +50.82287271986 11.6048 11.1391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176327_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176327_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:22.88 +43:33:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 4.014 387733605781953280 010.09411778026 +43.55860040144 11.2825 10.8794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176328_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176328_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 176329_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176329_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:00.59 +45:19:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 1.707 388281712328393088 009.25185782553 +45.32900631652 11.3565 10.9421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176331_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176331_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176333_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176333_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176335_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176335_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 176338_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176338_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:43.79 +41:05:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 3.951 381168284414660480 010.43117150584 +41.08465318952 11.3738 10.9080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176339_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176339_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:41.36 +41:03:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 4.095 381209065129717120 009.42104777427 +41.05218290861 10.8701 10.4146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176340_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176340_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 176342_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176342_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:12.01 +41:24:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.057 369271839182065792 011.54916079268 +41.40702191659 11.0531 10.6827 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176343_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176343_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:59.88 +46:01:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.563 389107789159219328 008.24865272008 +46.01600960878 11.1343 10.7286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176347_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176347_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:44.41 +41:40:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 4.366 381290673808228480 010.43434094101 +41.67332266630 11.1845 10.8156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176348_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176348_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176349_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176349_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176350_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176350_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176351_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176351_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:58:52.36 +48:39:12.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)
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Considering the candidate 176352_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176352_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176353_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176353_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:55:13.59 +50:47:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 4.183 403035710967313664 013.80803977024 +50.78735270696 11.6160 11.1891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176354_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176354_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176355_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176355_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:04.49 +42:00:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 2.884 381359668162559104 010.01774860401 +42.00516290543 11.1963 10.6884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176356_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176356_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (19.6") between the two second-epoch detections
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Considering the candidate 176357_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176357_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:50:20.33 +41:37:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 1.667 375062692047815680 012.58469177131 +41.63034266482 11.5740 11.1001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176358_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176358_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:33.29 +48:03:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 5.540 390495097953210112 009.89076751304 +48.05099340417 11.4442 11.0719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176361_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176361_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:09.43 +48:21:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 5.295 390928546056464896 008.29100352915 +48.36262690675 10.9444 10.2746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176364_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176364_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176365_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176365_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:33.16 +41:01:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 4.818 381175809197116032 009.88699858483 +41.03174265460 10.9359 10.5398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176366_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176366_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:23.54 +43:07:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 3.353 387475903447302656 010.84765758126 +43.11703872016 11.4380 11.0166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176367_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176367_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176368_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176368_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176369_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176369_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:09.79 +41:51:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 4.996 381448900395280256 009.53927676472 +41.85019207441 10.9904 10.6226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176370_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176370_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176373_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176373_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:22.62 +42:03:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 5.894 381323418641635328 010.84227485117 +42.05180003958 11.1822 10.7962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176374_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176374_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:40.17 +48:01:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 4.056 390867553223487616 009.41880648413 +48.03389959715 11.3361 10.7946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176375_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176375_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:19.08 +49:52:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 5.149 414723072893927040 010.57729349616 +49.87401558633 11.4264 11.0044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176376_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176376_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:54.18 +41:34:09.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
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Considering the candidate 176378_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176378_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:55.67 +49:44:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 3.740 414704415556002944 010.23349803505 +49.73527096498 11.4249 11.0455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176381_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176381_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176383_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176383_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:53.42 +43:20:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 5.234 387644820217992960 009.72063048333 +43.33469034127 11.0505 10.7490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176385_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176385_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:31.26 +45:44:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.621 388384752886913280 009.38020567569 +45.73803315018 11.3544 10.9909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176386_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176386_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176389_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176389_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:08.00 +43:40:14.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)
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Considering the candidate 176390_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176390_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176391_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176391_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:04.15 +41:04:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 3.709 381176904411012096 010.01785258006 +41.07158837098 11.0317 10.5022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176395_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176395_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176396_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176396_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:39.22 +45:26:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 4.930 388884279061587712 007.16534725424 +45.43803496851 10.7847 10.1347 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 176400_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176400_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:48:32.45 +50:21:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 5.864 414983249132240000 012.13311970513 +50.36379808892 11.4586 11.0277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176401_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176401_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:18.55 +44:37:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 4.001 387852043799926144 009.32797800719 +44.61805377079 11.2600 10.7608 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176402_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176402_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176403_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176403_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:10.92 +45:20:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 1.736 388279199770622080 009.29485886727 +45.34694972293 11.2900 10.8801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176404_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176404_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 176406_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176406_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 176407_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176407_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:00.36 +49:52:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.075 414758467724463616 011.50170419657 +49.87590708269 11.4751 11.1871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176408_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176408_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:29.86 +49:22:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 1.984 414542890428560000 012.37460635655 +49.37703721022 11.7283 11.3808 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176409_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176409_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:43.82 +49:42:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 5.267 414668582648149760 011.18159537342 +49.71339948363 11.3172 11.0581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176411_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176411_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:00.98 +49:39:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.133 414669987098163200 011.00499625561 +49.65906966568 11.2539 10.8459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176412_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176412_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176415_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176415_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:21.40 +41:00:17.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)
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Considering the candidate 176416_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176416_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:48:57.57 +41:12:20.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)
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Considering the candidate 176417_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176417_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:53:11.07 +50:31:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 3.058 414945036803773952 013.29737176946 +50.52963867496 11.5937 11.1477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176418_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176418_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176419_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176419_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176422_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176422_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176423_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176423_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 176424_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176424_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:12.59 +48:31:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 2.372 390567528285507712 010.80149041110 +48.52795852519 11.2952 10.9481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.372#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176425_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176425_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176428_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176428_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:25.14 +43:14:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.903 387632412055617920 009.85366446695 +43.23917615133 11.1072 10.6593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176431_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176431_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:39.07 +41:27:31.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)
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Considering the candidate 176433_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176433_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176436_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176436_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:52.11 +41:59:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 5.813 381366810686258816 010.46827079522 +41.99459397827 11.1377 10.6919 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 176440_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176440_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:30.84 +41:15:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.174 369266380282419712 011.12738194935 +41.26026157657 11.0445 10.6578 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176441_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176441_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:19.34 +46:00:35.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)
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Considering the candidate 176442_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176442_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:29.41 +41:06:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 3.228 375022151852704768 012.37250603222 +41.11256290286 11.2545 10.8277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176445_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176445_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176447_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176447_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:16.91 +50:22:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 5.713 414787570422600832 011.06913774523 +50.36937266450 11.1538 10.7143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176449_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176449_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:01.46 +41:47:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 5.632 381342557013130496 010.25430036367 +41.79292501318 10.8111 10.5121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176452_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176452_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:36.19 +47:43:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.448 390053644038270976 010.40090641237 +47.72301012785 11.2981 10.8316 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176453_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176453_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:45.07 +41:53:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 5.712 381446941890333696 009.68594928303 +41.89917403337 10.8338 10.4463 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176454_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176454_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:20.87 +42:20:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.222 381380730682305920 010.33712638015 +42.34382678901 11.0410 10.7713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176455_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176455_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176456_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176456_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:40.96 +43:21:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 3.816 387534074486308864 010.67040269839 +43.35448690906 12.6595 12.1798 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 176457_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176457_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:09.88 +41:48:34.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)
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Considering the candidate 176458_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176458_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:01.96 +42:45:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 4.395 387593383689645056 010.00832999786 +42.75363167645 11.2201 10.8032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176459_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176459_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:17.11 +41:52:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 4.514 381350081795577984 010.06988900707 +41.87416737121 10.7664 10.6554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176460_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176460_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:36.86 +48:00:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 3.608 390448673651930880 010.90481330421 +48.00948887789 11.3150 11.0348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176461_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176461_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:44.24 +47:05:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.593 389964789753937536 009.93437882770 +47.08818953086 11.5825 10.9754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176462_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176462_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:15.47 +48:44:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 4.316 390584845593594240 011.31626193106 +48.73876204845 11.4064 11.1615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176464_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176464_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176465_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176465_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:53:05.58 +50:55:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 4.808 415061486257684992 013.27175419699 +50.92602935733 11.2438 10.8351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176466_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176466_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:20.90 +48:32:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 2.944 390526743276117376 010.33618594161 +48.54293792799 11.1414 10.9185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176469_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176469_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:45.32 +46:16:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 5.670 389131737896646784 007.93722838987 +46.26960433327 10.7209 10.3107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176470_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176470_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176471_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176471_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:14.11 +49:42:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 4.654 391473972543173120 009.06037532899 +49.70378866547 10.7727 10.4866 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 176473_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176473_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:09.91 +41:20:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 2.461 369279127745334272 011.04072893564 +41.33640703220 11.0167 10.6161 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 176474_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176474_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:21.55 +44:12:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 5.409 387816206592763904 009.33769972496 +44.20211814176 10.9344 10.5131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176475_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176475_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:55.27 +49:07:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.645 414431603531008256 011.72961292816 +49.13028122439 11.3110 10.8477 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 176477_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176477_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:57.53 +42:34:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 2.303 375346503487484544 011.48991240194 +42.57012194496 11.2507 10.8394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176479_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176479_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176480_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176480_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:46.06 +42:00:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 4.858 375314759385465216 011.94337330727 +42.01252827057 11.2121 10.7829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176481_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176481_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176482_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176482_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:39.74 +46:01:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 2.602 389148058771324288 009.16643277308 +46.01813978395 10.9682 10.6297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176483_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176483_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176484_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176484_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:27.89 +48:56:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 5.857 390593637387756288 011.36797896611 +48.93436233815 11.3349 10.9228 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 176485_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176485_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176486_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176486_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:32.02 +41:06:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 2.912 375207518344841344 011.88245110313 +41.10550747273 10.9116 10.5438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176487_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176487_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:55:26.59 +50:48:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 5.176 403059075589403392 013.85994281346 +50.80566715381 11.2369 10.9598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176488_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176488_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:11.07 +49:27:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.660 391427999213585408 009.79714956167 +49.45412474007 10.9227 10.5049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176489_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176489_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:58.97 +50:41:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 4.967 414856015021012480 010.24391954654 +50.68959267555 10.7322 10.2782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176492_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176492_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176494_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176494_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:12.62 +44:42:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 3.489 388601292255765120 008.30122343417 +44.70023555336 10.6183 10.2896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176495_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176495_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176496_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176496_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176498_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176498_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:47.19 +46:35:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 2.670 389926135048367744 009.94601943139 +46.59958612922 10.9793 10.5617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176501_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176501_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176502_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176502_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176504_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176504_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176505_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176505_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:44.95 +47:25:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 3.618 389471757570628992 007.68615100260 +47.42357866107 10.5929 10.2264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176506_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176506_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176508_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176508_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:13.98 +41:35:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 2.817 381333790980072448 010.05840097319 +41.59177445017 10.6688 10.0509 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 176510_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176510_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 176511_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176511_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176512_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176512_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:31.06 +42:12:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 5.316 381518788104079616 008.87752066927 +42.20273851219 10.5080 10.1238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176513_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176513_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176514_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176514_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:52.97 +42:54:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 3.810 387601492587892736 009.96943401652 +42.91200094581 10.6142 10.3031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176517_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176517_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176519_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176519_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176521_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176521_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176523_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176523_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:38.07 +42:22:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 2.990 381391863237525632 010.15754414983 +42.37300624793 11.0721 10.4080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176524_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176524_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176525_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176525_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176527_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176527_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176528_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176528_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176530_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176530_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:09.60 +41:26:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 4.539 381238103402939648 010.03861929781 +41.43786320776 10.6958 10.1564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176533_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176533_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176534_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176534_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176535_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176535_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176536_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176536_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:45.73 +49:16:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.319 414456686139982848 011.94045680278 +49.27219539373 11.0638 10.7179 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 176538_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176538_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176540_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176540_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:50.51 +48:17:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 3.904 390892193453530880 009.20935745705 +48.29810535948 10.5416 10.2337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176541_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176541_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176543_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176543_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176545_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176545_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176546_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176546_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176547_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176547_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176548_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176548_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176549_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176549_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176550_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176550_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176551_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176551_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:43.84 +41:24:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 5.181 381413196331782528 009.18097505489 +41.40959833773 9.5168 9.3246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176552_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176552_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176553_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176553_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176554_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176554_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176556_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176556_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 176557_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176557_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176559_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176559_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176560_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176560_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176561_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176561_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:39.71 +41:22:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 3.937 369259675834685184 010.91420222510 +41.37555637118 10.4802 10.0648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176562_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176562_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176563_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176563_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:29.31 +49:24:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 3.556 414637727600073984 010.87102683079 +49.41512326272 10.7885 10.3032 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 176564_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176564_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:34.57 +49:54:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.555 414573852848977152 011.89359504252 +49.90951661559 10.8507 10.6239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176565_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176565_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:47:59.22 +49:10:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 0.404 414443010964331648 011.99658699174 +49.18315942043 10.9257 10.6482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176567_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176567_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176568_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176568_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176569_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176569_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176570_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176570_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:39.56 +50:00:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 4.364 414725585453928832 010.66305600531 +50.01165584887 10.7035 10.3195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176572_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176572_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:33.66 +46:09:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 4.564 388422930853127936 009.38908931562 +46.16440838283 10.6140 10.1752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176573_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176573_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176575_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176575_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176579_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176579_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176580_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176580_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176581_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176581_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176583_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176583_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 176585_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176585_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:47.71 +43:44:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 2.847 387740168491957376 009.94778503848 +43.73485611640 10.4131 10.1178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.847#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176586_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176586_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176587_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176587_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176588_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176588_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 176589_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176589_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:24.84 +42:53:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 5.302 387433164229245312 010.35193655743 +42.88546305719 10.2632 9.9391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176590_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176590_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:43.23 +47:10:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.028 390056942573069824 010.18042792855 +47.17686454392 10.5466 10.2221 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 176591_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176591_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:44.15 +41:03:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 2.161 369237586821696128 011.18322801254 +41.05667745431 10.3255 9.8031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176592_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176592_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176593_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176593_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176594_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176594_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:52:59.20 +49:30:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 1.419 414509978093147136 013.24636708681 +49.50671275394 10.8069 10.5346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176595_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176595_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176596_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176596_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:04.19 +47:32:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 2.683 390047287486701568 010.51647518370 +47.53403344305 10.5697 10.1771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176597_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176597_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176599_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176599_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 176601_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176601_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (18.5") between the two second-epoch detections
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Considering the candidate 176603_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176603_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:04.68 +49:37:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 1.672 414658309086675840 011.51905513083 +49.62861417770 10.5219 10.2649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176604_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176604_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:15.29 +43:32:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 3.709 387654956340730240 009.81232134836 +43.54027503966 10.1503 9.8486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176606_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176606_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176607_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176607_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176609_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176609_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176610_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176610_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176611_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176611_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176613_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176613_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176614_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176614_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176615_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176615_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176616_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176616_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176617_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176617_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:12.14 +42:38:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 5.284 387403855372450560 010.04889298553 +42.63599814752 9.9499 9.7059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176618_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176618_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:46:06.99 +41:18:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 3.762 369224049084752256 011.52831396319 +41.30887318038 10.1446 9.7516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176619_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176619_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176620_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176620_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176622_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176622_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:48.26 +43:27:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.25, MAG_FAINT_SEARCH_LIMIT=12.23)GAIADR2_OUTPUT=# 4.820 387547410359410432 010.44952874743 +43.46005710791 10.0889 9.7253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176623_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176623_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176624_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176624_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:30.14 +49:28:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 1.605 414652777168831360 011.37500457655 +49.47648264162 10.3715 10.0501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176625_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176625_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:18.44 +49:41:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 2.363 414668994965012864 011.07604198974 +49.68996629398 10.2236 9.8122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176626_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176626_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:15.93 +49:05:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.16, MAG_FAINT_SEARCH_LIMIT=12.14)GAIADR2_OUTPUT=# 5.559 391352613947076352 008.31467176528 +49.09923480650 9.6289 9.3690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176627_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176627_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:03.12 +49:14:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 2.219 391401503555858816 009.76225549393 +49.24710124154 10.0050 9.6003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176628_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176628_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:54:01.70 +50:35:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.09, MAG_FAINT_SEARCH_LIMIT=12.07)GAIADR2_OUTPUT=# 3.185 415036502427305088 013.50600332428 +50.59239247377 10.2936 9.9193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176629_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176629_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:07.06 +41:23:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 5.016 381245834344063744 009.52822253875 +41.39090498107 9.6983 9.2957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176631_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176631_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:04.50 +45:26:56.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.15, MAG_FAINT_SEARCH_LIMIT=12.13)
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Considering the candidate 176632_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176632_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176633_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176633_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176634_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176634_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 176635_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176635_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176636_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176636_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176639_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176639_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:34.86 +42:09:26.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176640_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176640_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176641_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176641_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176642_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176642_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176644_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176644_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176645_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176645_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:22.12 +42:55:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 5.101 387598434571174656 009.84033395583 +42.93015570535 9.6832 9.3541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176646_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176646_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176647_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176647_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:50:30.11 +50:34:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 4.090 415000974457835008 012.62397192504 +50.57643754899 10.0846 9.7018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176648_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176648_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:45.20 +42:24:48.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176649_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176649_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 176651_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176651_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:23.20 +45:53:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 2.193 388401181138899712 009.84620863932 +45.89131437776 9.8372 9.5176 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176653_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176653_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176654_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176654_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:50.95 +42:59:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 4.507 387423818380396416 010.46072417970 +42.99377462728 9.5785 9.1866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176655_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176655_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 176656_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176656_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176657_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176657_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176658_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176658_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:11.58 +49:53:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.59, MAG_FAINT_SEARCH_LIMIT=11.57)GAIADR2_OUTPUT=# 1.300 414677138223228800 011.29875499725 +49.88562894583 9.6991 9.2647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176659_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176659_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176660_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176660_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:40:58.26 +41:43:54.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176661_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176661_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:52.16 +46:23:06.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176662_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176662_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:20.00 +41:55:36.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176663_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176663_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:55.83 +42:23:42.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176664_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176664_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:53.03 +43:27:47.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176665_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176665_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176666_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176666_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:31.65 +40:57:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 5.722 369246898310562432 010.63002747883 +40.95351657081 9.1294 8.6470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176667_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176667_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:35:10.07 +44:50:13.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)
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Considering the candidate 176668_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176668_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:52:57.37 +50:46:09.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176671_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176671_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:42.25 +45:46:51.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176672_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176672_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176673_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176673_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176674_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176674_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:02.20 +43:22:36.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176675_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176675_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:37.31 +43:38:13.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176678_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176678_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176679_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176679_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 176680_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176680_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176681_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176681_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:45.31 +42:31:33.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176682_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176682_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176683_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176683_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:11.00 +49:59:16.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176684_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176684_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:02.78 +50:15:16.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176685_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176685_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176686_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176686_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:07.12 +51:01:40.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176687_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176687_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:02.53 +50:29:41.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176688_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176688_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:38.29 +50:35:12.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176690_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176690_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:08.17 +49:28:06.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176692_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176692_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:11.54 +49:23:27.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176693_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176693_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:25:48.19 +49:39:32.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176694_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176694_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:25:03.35 +50:43:48.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176695_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176695_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:09.49 +45:56:59.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176696_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176696_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:38.58 +50:13:30.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176697_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176697_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:03.88 +48:02:23.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176698_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176698_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:41:54.86 +49:37:19.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.10, MAG_FAINT_SEARCH_LIMIT=11.08)
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Considering the candidate 176699_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176699_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:37:20.96 +50:18:30.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176700_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176700_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:33.91 +50:23:14.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176701_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176701_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:16.52 +50:07:51.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176702_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176702_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:54.00 +45:00:13.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176704_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176704_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:46.96 +50:15:35.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176705_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176705_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:04.78 +50:00:14.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 176708_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176708_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:33:22.81 +49:51:25.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176709_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176709_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176711_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176711_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176715_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176715_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176717_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176717_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176718_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176718_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176720_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176720_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176723_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176723_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:17.80 +49:47:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 5.311 391629141122749056 007.07254507902 +49.78784479422 9.1008 8.4598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176726_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176726_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:44.89 +50:01:27.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)
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Considering the candidate 176727_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176727_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176728_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176728_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176730_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176730_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176732_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176732_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176733_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176733_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:38.81 +50:24:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)GAIADR2_OUTPUT=# 3.550 391706965928784000 007.66298540288 +50.40727660935 9.4173 9.0957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176734_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176734_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:48.10 +49:14:57.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)
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Considering the candidate 176736_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176736_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:23.93 +50:20:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 2.024 391703014558914944 007.85019977732 +50.33429986706 9.4211 9.0333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176739_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176739_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176740_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176740_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176741_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176741_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176742_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176742_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176743_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176743_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176745_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176745_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176747_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176747_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:17.96 +50:29:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.86, MAG_FAINT_SEARCH_LIMIT=11.84)GAIADR2_OUTPUT=# 4.878 394678494883219456 006.57675961062 +50.48489476133 9.2073 8.4242 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176749_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176749_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:15.53 +50:51:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 4.635 415761802144526336 007.81641117540 +50.86387439431 9.4737 8.7586 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 176753_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176753_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176754_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176754_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:56.22 +49:47:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 4.382 391638005936051968 007.48311254746 +49.79122061574 9.6498 9.5100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176756_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176756_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:27.54 +50:58:07.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176758_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176758_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176761_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176761_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176762_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176762_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176770_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176770_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176771_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176771_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176772_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176772_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176775_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176775_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176776_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176776_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176777_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176777_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176778_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176778_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176781_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176781_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:25.59 +49:59:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 5.057 391691293589856512 007.85850924810 +49.98818341604 9.8375 9.3817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176783_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176783_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176787_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176787_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176788_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176788_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:39.68 +49:53:27.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)
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Considering the candidate 176789_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176789_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176791_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176791_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:25:16.58 +50:31:59.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176793_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176793_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176794_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176794_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:38:28.78 +50:21:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 4.302 415510976054427776 009.62166270923 +50.35728985848 10.2602 9.8882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176797_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176797_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176798_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176798_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 176799_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176799_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176800_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176800_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176801_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176801_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:10.01 +50:45:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 5.557 394775771601571072 006.54378997895 +50.75272278238 9.7045 8.9763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176803_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176803_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176804_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176804_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176805_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176805_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176806_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176806_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176807_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176807_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176808_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176808_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:44.61 +50:02:57.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176811_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176811_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:49.82 +50:46:16.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 176812_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176812_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176814_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176814_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:25:48.04 +49:44:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 4.554 394256424156489472 006.45087879692 +49.74015509740 9.8639 9.1166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176815_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176815_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176816_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176816_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176819_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176819_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176822_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176822_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176825_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176825_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176826_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176826_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176827_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176827_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:54.64 +50:11:41.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)
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Considering the candidate 176830_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176830_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176831_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176831_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176832_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176832_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:33.30 +49:40:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 3.129 391610552499466368 007.13993701135 +49.66896214427 10.2596 9.8417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176835_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176835_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176836_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176836_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176838_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176838_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176840_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176840_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176841_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176841_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:35.34 +49:42:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 2.102 391613954114031488 007.39736374143 +49.70619046947 10.4307 10.2644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176842_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176842_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176845_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176845_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:52.32 +50:05:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 3.592 391649138485878528 007.46752916349 +50.09671582449 11.3411 11.1406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176849_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176849_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176852_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176852_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:29.98 +50:25:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 5.102 415537849665419392 009.12642736672 +50.42212630779 10.6344 10.2258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176854_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176854_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176859_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176859_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:36.12 +49:48:43.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)
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Considering the candidate 176864_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176864_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176865_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176865_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176867_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176867_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176868_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176868_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176872_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176872_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176873_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176873_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176874_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176874_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176875_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176875_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:11.61 +50:35:32.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)
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Considering the candidate 176884_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176884_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176885_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176885_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176886_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176886_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176887_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176887_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176889_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176889_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:59.27 +50:36:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 5.692 391773692540525952 006.99929612938 +50.60628650053 10.2568 9.5520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.692#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176892_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176892_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:04:53.15 +45:01:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.642 376945163331289728 016.22135096508 +45.02708864661 12.4963 10.8056 VARIABLE#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 176896_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176896_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:00.19 +49:32:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 3.450 391608697073672192 007.25106134669 +49.53494226604 10.4453 10.0090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176898_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176898_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176900_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176900_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176901_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176901_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 176902_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176902_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176903_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176903_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176904_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176904_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176905_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176905_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176906_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176906_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176908_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176908_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176909_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176909_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176910_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176910_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176917_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176917_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176918_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176918_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176919_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176919_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176921_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176921_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176925_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176925_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:15.13 +49:55:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 3.852 391599248149470080 007.56412495568 +49.91767239271 10.7234 10.4820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176926_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176926_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176931_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176931_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176936_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176936_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176937_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176937_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176941_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176941_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176942_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176942_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176947_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176947_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176952_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176952_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176955_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176955_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176956_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176956_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176957_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176957_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:34.49 +49:30:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 5.255 391608112962947712 007.14449263950 +49.51595140230 10.7099 10.3230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 176960_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176960_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176963_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176963_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176965_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176965_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176966_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176966_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176967_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176967_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176968_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176968_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176969_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176969_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176970_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176970_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176972_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176972_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:50.99 +50:41:17.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)
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Considering the candidate 176973_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176973_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176976_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176976_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176980_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176980_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176983_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176983_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 176984_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176984_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176985_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176985_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176986_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176986_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176989_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176989_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176990_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176990_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176993_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176993_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176994_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 176994_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 176995_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176995_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176996_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176996_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 176997_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 176997_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177002_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177002_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177005_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177005_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177007_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177007_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177009_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177009_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177010_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177010_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177012_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177012_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177013_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177013_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177014_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177014_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177015_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177015_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177021_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177021_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177022_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177022_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177023_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177023_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177026_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177026_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:54.58 +49:20:19.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)
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Considering the candidate 177027_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177027_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177028_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177028_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:49:44.20 +41:02:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.919 375009297014343808 012.43480978931 +41.04180445710 11.4992 10.9829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177029_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177029_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177035_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177035_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:44.75 +49:33:45.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)
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Considering the candidate 177036_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177036_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177038_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177038_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177040_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177040_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:21.27 +49:48:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 5.621 391627216977377280 006.83694996965 +49.81154334333 10.8694 10.1481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177041_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177041_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177042_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177042_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 177044_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177044_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177046_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177046_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177047_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177047_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:34.08 +49:57:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 4.579 391690438894780032 007.89339750506 +49.95690588784 11.2626 11.2187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177049_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177049_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177050_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177050_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177052_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177052_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177057_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177057_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177060_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177060_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177061_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177061_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177064_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177064_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177069_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177069_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177070_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177070_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177075_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177075_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177078_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177078_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177079_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177079_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:58:40.67 +49:13:55.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177081_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177081_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177082_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177082_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177085_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177085_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177086_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177086_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177090_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177090_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:42.80 +50:42:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 2.862 394772610505659904 006.67946570684 +50.71087873965 10.7674 9.9253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177091_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177091_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177098_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177098_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177099_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177099_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:39:44.48 +45:52:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.356 350663365094201728 024.93604373749 +45.87115084105 13.0686 12.5919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177100_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177100_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177101_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177101_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177102_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177102_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177103_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177103_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177104_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177104_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177105_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177105_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177108_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177108_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177110_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177110_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177116_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177116_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177120_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177120_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177122_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177122_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177129_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177129_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177133_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177133_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177136_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177136_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177138_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177138_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:17.49 +50:32:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 4.429 394679083297696256 006.57476560449 +50.55012613488 11.0307 10.0138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177141_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177141_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177142_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177142_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177144_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177144_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177148_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177148_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177154_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177154_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177155_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177155_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 177156_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177156_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177157_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177157_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177158_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177158_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177159_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177159_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177160_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177160_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177163_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177163_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177165_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177165_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177166_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177166_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177169_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177169_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177172_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177172_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177175_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177175_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:01.71 +50:54:08.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)
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Considering the candidate 177184_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177184_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:34.48 +49:33:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.698 394250239403705600 006.64308936859 +49.56151217338 10.9816 10.5738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177186_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177186_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177191_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177191_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 177197_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177197_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177202_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177202_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177205_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177205_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:36.81 +50:19:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.867 391705179222421504 007.65458770060 +50.33053574658 11.3879 10.9591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177208_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177208_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:50:43.67 +46:30:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.301 378110645657223680 012.68038516463 +46.50846733779 12.9318 11.0010 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177209_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177209_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:46.25 +50:25:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 5.816 391727032016242688 007.94111281171 +50.43046636161 11.2641 10.5704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177211_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177211_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177215_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177215_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177216_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177216_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177217_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177217_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177219_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177219_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177220_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177220_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177222_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177222_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177223_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177223_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177226_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177226_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177230_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177230_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177231_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177231_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177232_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177232_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177233_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177233_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177235_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177235_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177239_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177239_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177242_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177242_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:06.30 +49:47:15.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)
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Considering the candidate 177243_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177243_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177244_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177244_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177245_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177245_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177246_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177246_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177252_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177252_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177254_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177254_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177259_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177259_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177262_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177262_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177273_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177273_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:51.59 +49:20:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.682 391235820899200128 006.96419133878 +49.33553391032 11.2026 10.7053 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 177274_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177274_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177281_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177281_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177283_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177283_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177284_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177284_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177289_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177289_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177293_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177293_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:48:51.61 +42:15:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.629 347613903953683840 027.21500747494 +42.26722978280 13.3467 12.8836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177296_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177296_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:56.84 +49:58:55.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 177299_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177299_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177303_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177303_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177306_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177306_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177310_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177310_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177317_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177317_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177318_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177318_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177319_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177319_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177328_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177328_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177332_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177332_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177336_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177336_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177339_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177339_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177343_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177343_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177344_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177344_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177345_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177345_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:19.25 +50:47:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.724 391788467227978752 007.58210828561 +50.79383251859 11.6325 10.9107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177349_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177349_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177354_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177354_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:42.54 +46:11:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.337 389679569565005312 011.42584313954 +46.19939545252 13.4806 11.7240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177357_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177357_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177359_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177359_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177361_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177361_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177362_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177362_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:51.61 +48:58:09.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 177367_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177367_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177369_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177369_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:48:39.79 +50:59:07.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177371_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177371_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177374_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177374_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:28:26.31 +43:54:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.689 396588179080323840 022.10983810811 +43.91647102856 13.7323 13.3025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177375_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177375_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:29:04.53 +49:33:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 5.792 391606257537072128 007.26989418299 +49.56366126868 11.9686 11.7828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177377_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177377_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:46.47 +50:44:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 5.543 391740535392992384 007.69556519593 +50.74487649924 11.4288 10.6908 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 177379_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177379_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177381_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177381_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:40:40.06 +44:48:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.437 350476929153787904 025.16658293239 +44.81138415104 13.5352 13.0049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177382_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177382_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177388_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177388_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177390_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177390_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177393_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177393_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177396_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177396_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:37:34.13 +48:23:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.420 399376025171399936 024.39160544529 +48.39165104590 13.4967 13.0118 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177400_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177400_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177402_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177402_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177403_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177403_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177407_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177407_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177412_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177412_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:29.63 +49:41:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 5.882 391616634178019968 007.12300842627 +49.68969098300 11.2714 10.8496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177416_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177416_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:28:18.73 +49:44:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 5.782 391628625726686848 007.07857570483 +49.74542968425 11.3786 10.8147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177417_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177417_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:58:32.43 +49:10:20.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177420_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177420_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:29.85 +49:35:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.766 394250273763427840 006.62439426961 +49.59140707086 11.4545 11.0592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177422_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177422_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:58.69 +50:26:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.064 391729952593745792 007.74513568324 +50.43326381799 11.6493 11.2169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177423_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177423_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177425_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177425_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177426_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177426_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177429_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177429_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177433_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177433_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177436_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177436_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177443_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177443_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:47:51.21 +49:50:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.716 357856026565461376 026.96367957821 +49.84894789411 13.3502 12.8426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177444_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177444_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177453_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177453_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177456_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177456_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:26:01.45 +50:42:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 4.599 394774839589681280 006.50756836559 +50.70658179787 11.2457 10.4551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177459_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177459_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177463_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177463_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:45.81 +42:47:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.935 382353557947860224 007.69195689135 +42.78987943784 11.9117 11.4468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177464_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177464_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177465_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177465_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 177469_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177469_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177477_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177477_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177482_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177482_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:54:46.52 +50:16:08.1 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 177484_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177484_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:51:23.24 +42:44:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.520 349135593687015680 027.84663571811 +42.74870213469 13.4142 13.0181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177485_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177485_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177487_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177487_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:38:06.07 +46:00:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.175 350679823408838912 024.52670473586 +46.00717325474 13.7192 13.0422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177491_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177491_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:27:07.54 +50:39:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.204 394771510994048384 006.78143661172 +50.65816622521 11.2684 10.8092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177497_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177497_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177498_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177498_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177506_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177506_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:58:44.99 +48:26:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.908 356741740250042368 029.68923869171 +48.44662586974 13.1984 12.4084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177511_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177511_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177514_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177514_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177515_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177515_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:31:30.17 +50:17:03.7 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 177522_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177522_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177523_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177523_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177525_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177525_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177530_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177530_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177533_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177533_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177541_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177541_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177550_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177550_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 177555_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177555_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177559_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177559_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177560_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177560_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:40:43.01 +40:33:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.572 347218045407981056 025.17975314194 +40.55011100069 13.5106 12.9468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177564_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177564_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177574_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177574_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 177586_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177586_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:53:54.45 +46:07:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.475 350084059904735232 028.47722962544 +46.12032789309 13.6800 13.2636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177592_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177592_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:39:23.46 +45:08:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 4.623 350497716795383040 024.84708495952 +45.14477864438 14.1423 13.5703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177596_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177596_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177604_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177604_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177606_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177606_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177609_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177609_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:45:59.85 +45:34:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 3.394 350790908442913536 026.50020834597 +45.57635171405 13.8129 13.0621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177629_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177629_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177631_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177631_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177634_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177634_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:30:41.71 +50:38:30.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 177638_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177638_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:40:07.83 +42:43:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.401 348573846324395392 025.03227712054 +42.72346004746 13.9059 13.5271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177646_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177646_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 177647_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177647_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177665_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 177665_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 177690_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177690_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:34:57.25 +50:50:18.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)
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Considering the candidate 177695_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177695_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177713_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177713_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177722_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177722_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 177760_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177760_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:32:01.21 +42:39:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.446 382302602455906816 008.00514375264 +42.66032339134 14.4052 13.8896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177806_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 177806_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 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 26768_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 26768_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 04656_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 04656_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 106955_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 106955_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 73358_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 73358_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:33:35.61 +46:31:13.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 77883_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 77883_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:25:48.55 +46:24:13.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 136118_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 136118_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 27694_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 27694_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 18245_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 18245_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 122338_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 122338_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (32.8") between the two second-epoch detections
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Considering the candidate 30387_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 30387_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 132140_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 132140_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:33:58.41 +43:22:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.380 348838141431819392 023.49375933315 +43.37718691662 13.7737 13.2471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 14617_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 14617_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 138895_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 138895_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:55:57.95 +44:13:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.257 377282094924322560 013.99097509286 +44.22834956168 13.5594 12.9758 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 49356_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 49356_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 16201_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 16201_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 45996_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 45996_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 70664_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 70664_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 43529_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 43529_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 73227_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 73227_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 29056_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 29056_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 60354_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 60354_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 37891_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 37891_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:10:12.95 +49:10:14.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 65856_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 65856_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 45019_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 45019_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 07496_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 07496_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 27651_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 27651_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 125047_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 125047_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 37056_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 37056_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (32.0") between the two second-epoch detections
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Considering the candidate 92851_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 92851_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
Rejecting candidate due to large distance (34.3") between the two second-epoch detections
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Considering the candidate 53187_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 53187_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 164137_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 164137_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 94276_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 94276_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 11234_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 11234_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 116201_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 116201_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 91655_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 91655_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27968_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 27968_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 163925_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 163925_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83561_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 83561_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:15:42.26 +46:12:18.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 70545_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 70545_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163782_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 163782_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51463_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 51463_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 62909_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 62909_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33481_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 33481_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:58:20.74 +49:25:07.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124529_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 124529_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
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Considering the candidate 84295_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 84295_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59073_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 59073_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134182_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 134182_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86925_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 86925_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:31:58.33 +45:46:20.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16232_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 16232_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22005_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 22005_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:26:27.57 +49:53:57.1 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64104_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 64104_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:16:19.80 +47:27:30.8 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163483_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 163483_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67580_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 67580_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16328_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 16328_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:45:56.30 +50:23:15.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58599_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 58599_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:14:04.53 +47:52:07.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91269_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 91269_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131343_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 131343_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87894_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 87894_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42080_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 42080_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23345_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 23345_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47085_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
Preparing report for the candidate 47085_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83170_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 83170_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:11:10.58 +46:11:02.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 94772_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 94772_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:12:34.12 +45:20:19.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 141941_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 141941_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:17:41.70 +44:37:57.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 66550_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 66550_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:09:30.31 +47:14:31.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 65634_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 65634_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:03:01.84 +47:22:34.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62812_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 62812_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:18:10.05 +47:25:11.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100557_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 100557_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:17:04.99 +44:54:10.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90705_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 90705_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:22:20.12 +45:31:50.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 135079_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 135079_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:08:01.40 +43:56:38.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89683_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 89683_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:57:39.83 +45:50:22.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145303_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 145303_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:00:03.69 +44:42:47.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90630_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 90630_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 01:27:39.75 +45:24:27.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47191_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 47191_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:55:05.29 +48:40:42.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69328_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 69328_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:43:28.16 +47:01:31.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52374_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 52374_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:44:43.94 +48:17:07.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143546_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 143546_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:36:46.57 +44:29:21.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15223_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 15223_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:42:03.98 +50:30:49.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35334_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 35334_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:39:09.94 +49:21:19.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08897_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083
The candidate 08897_And-02-Q2b1x1_2026-02-21_21-38-33_20.00sec_-15.00C_LIGHT_0083 did not pass the final checks
**** FOUND 00:48:50.25 +50:58:08.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 107s
make_report_in_HTML.sh TOTAL: 1294s
Prepared the HTML report for the field And-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:45:56.25 +50:23:15.7
01:26:27.60 +49:53:58.1
00:58:20.83 +49:25:06.4
01:10:12.93 +49:10:15.4
01:14:04.52 +47:52:07.5
01:16:19.81 +47:27:31.0
01:33:35.62 +46:31:13.7
01:25:48.53 +46:24:13.0
01:15:42.26 +46:12:18.4
00:29:32.62 +49:25:24.8
00:44:52.14 +46:14:18.9
00:34:34.69 +42:09:25.3
00:54:37.50 +49:28:21.1
00:38:39.17 +43:48:36.1
00:33:45.23 +42:24:49.0
00:35:55.68 +42:23:43.1
00:40:58.52 +41:43:55.5
00:42:32.09 +40:57:18.8
00:39:19.95 +41:55:34.6
00:46:22.18 +50:04:38.5
00:52:57.44 +50:46:08.6
00:33:22.70 +49:51:24.6
00:34:27.80 +49:19:12.3
00:40:15.19 +50:49:23.2
00:42:38.80 +49:34:51.5
00:28:11.05 +50:28:08.9
00:33:55.33 +48:39:10.4
00:35:43.70 +41:45:08.4
00:28:05.04 +49:10:14.5
00:31:28.44 +49:04:22.2
00:36:27.59 +50:58:06.8
00:25:16.24 +50:31:57.6
00:46:51.43 +42:18:06.4
00:32:50.53 +49:19:44.5
00:26:49.68 +50:46:16.7
00:55:15.09 +49:39:22.0
00:36:48.66 +50:42:52.3
00:31:44.18 +50:02:56.2
01:31:58.34 +45:46:20.7
00:38:56.24 +50:58:31.5
01:12:32.83 +50:51:24.3
00:54:54.46 +41:10:28.6
00:35:44.05 +50:33:08.7
00:57:28.45 +42:47:54.3
01:36:40.37 +42:51:19.4
01:11:45.37 +43:16:18.1
01:21:37.14 +43:32:51.2
00:54:27.34 +43:55:38.0
01:20:28.68 +43:52:02.2
01:17:55.72 +50:24:13.4
01:10:12.11 +50:22:50.0
01:00:48.10 +50:23:41.6
01:35:12.12 +46:33:47.6
00:51:23.98 +49:09:52.9
00:43:46.56 +51:02:35.7
00:32:18.61 +50:27:38.4
00:40:54.80 +43:18:07.5
00:41:27.98 +44:06:28.9
01:00:20.71 +41:01:19.8
00:45:14.07 +41:03:01.6
00:29:49.36 +41:44:42.3
00:44:05.02 +42:19:57.0
01:29:26.69 +46:27:24.0
01:28:47.66 +44:16:39.2
00:56:54.71 +41:31:41.7
00:46:26.17 +45:54:34.7
00:32:49.44 +41:33:51.5
00:42:36.20 +44:15:33.5
01:51:23.52 +49:56:14.5
00:39:05.16 +40:55:41.8
00:30:50.10 +41:16:32.5
00:40:06.38 +42:22:42.1
00:32:34.15 +48:41:56.2
00:42:10.50 +41:26:20.5
00:39:18.12 +49:31:27.4
00:46:32.24 +41:51:49.3
00:31:15.32 +44:21:00.0
00:31:08.32 +42:49:07.5
00:29:18.89 +46:12:00.8
00:38:14.08 +42:16:52.0
01:21:11.80 +48:29:08.2
00:40:19.55 +43:04:59.3
00:30:51.74 +41:44:46.9
00:43:44.55 +41:04:55.1
00:36:25.74 +42:34:30.4
00:49:17.74 +42:47:31.3
00:40:33.46 +44:20:49.8
00:30:55.16 +50:04:24.3
00:40:14.45 +44:46:47.0
00:42:21.35 +45:04:14.7
00:39:07.27 +48:10:19.6
01:19:23.91 +48:26:38.1
00:36:25.84 +41:03:26.3
00:31:05.63 +46:50:59.2
00:45:08.14 +46:22:02.1
00:45:46.38 +42:25:21.5
00:45:32.07 +42:27:42.3
00:42:59.97 +41:05:53.6
00:35:36.91 +43:02:35.6
00:38:24.78 +44:16:41.4
00:37:27.73 +42:03:43.4
00:33:09.14 +42:48:18.3
00:36:54.15 +48:50:38.7
00:38:17.33 +43:36:12.0
00:35:46.84 +41:39:44.1
00:35:38.15 +41:02:02.2
00:54:44.06 +41:23:44.1
00:38:32.84 +43:35:18.0
00:40:04.02 +42:13:37.6
00:49:57.43 +45:10:25.3
00:42:19.61 +42:25:25.9
00:35:02.82 +42:35:09.7
00:33:09.09 +42:48:22.6
00:36:49.40 +44:35:15.5
00:37:34.52 +44:27:48.1
00:41:27.25 +42:12:52.2
00:32:54.83 +41:50:09.4
00:32:55.07 +40:52:22.6
00:35:44.15 +41:15:09.3
00:40:38.56 +43:06:25.1
00:43:11.12 +41:36:14.9
00:33:27.98 +44:19:03.1
01:10:43.33 +43:20:57.2
00:45:35.47 +43:34:46.5
00:44:52.33 +41:25:03.3
00:37:48.84 +43:51:08.4
00:35:00.04 +42:13:42.7
00:36:28.24 +44:27:45.7
00:40:45.58 +42:16:48.8
00:29:04.68 +46:31:28.9
00:46:37.44 +41:08:56.1
00:44:53.46 +49:53:06.5
00:43:00.26 +41:28:54.6
00:31:24.11 +44:25:24.4
00:42:30.39 +44:32:12.6
00:41:21.83 +46:23:45.3
00:39:41.74 +41:26:54.8
00:32:54.29 +47:07:43.0
00:27:31.57 +48:49:15.5
00:42:24.39 +43:09:57.8
00:55:13.37 +46:39:01.7
00:47:20.19 +43:53:19.0
00:33:35.66 +45:30:31.1
01:11:14.09 +50:23:29.3
00:35:45.77 +49:23:12.7
00:44:08.79 +42:27:38.3
00:40:42.40 +48:48:37.5
00:33:28.11 +42:03:50.7
00:38:45.74 +43:49:49.7
00:42:52.87 +43:18:59.8
00:40:46.85 +50:18:46.7
00:39:18.67 +48:30:25.9
00:38:48.42 +46:30:21.2
00:30:50.61 +43:43:00.9
00:36:22.78 +50:38:17.7
01:07:07.67 +43:02:44.6
00:51:35.56 +41:37:04.6
00:36:34.59 +49:09:03.9
00:27:53.38 +46:08:08.5
00:37:30.07 +45:50:30.3
00:55:48.81 +44:10:48.4
00:29:05.57 +45:41:25.8
00:35:25.34 +49:55:43.8
00:36:29.53 +49:32:09.7
00:40:55.67 +40:57:43.4
00:41:18.74 +44:10:21.0
00:34:28.88 +42:30:06.4
00:51:55.88 +51:02:22.0
00:33:59.04 +50:30:22.6
00:43:25.55 +41:24:23.1
00:28:39.06 +46:42:07.2
00:46:38.86 +42:57:47.0
00:33:55.78 +46:08:48.1
00:36:00.05 +46:04:24.3
00:38:51.55 +43:44:31.9
00:45:30.88 +40:58:40.2
00:42:11.80 +48:53:19.9
00:30:44.42 +47:48:53.3
00:39:02.12 +49:30:32.7
00:34:35.69 +47:34:42.4
00:49:36.89 +41:29:06.4
00:32:50.08 +42:34:54.4
00:39:25.42 +47:25:28.8
00:34:42.75 +43:33:40.6
00:37:33.86 +41:55:06.5
00:32:04.48 +43:46:41.9
00:36:05.33 +44:20:32.8
00:52:35.41 +44:54:12.9
00:35:45.81 +42:25:30.9
00:30:30.05 +44:28:06.2
00:38:46.51 +46:52:37.6
01:03:40.80 +48:10:46.9
00:47:55.32 +49:51:36.5
00:40:03.46 +41:19:01.0
00:33:39.87 +44:07:45.0
00:46:17.98 +50:52:33.5
00:27:54.37 +49:29:44.4
00:36:36.31 +41:42:11.7
00:39:40.36 +42:36:07.8
00:34:59.13 +43:38:26.1
01:13:46.30 +46:34:07.8
00:37:41.55 +47:58:23.2
00:47:49.56 +48:00:39.9
00:37:40.43 +46:38:53.5
00:28:53.47 +44:15:58.5
01:05:51.98 +48:50:26.6
00:34:14.62 +42:15:49.1
00:36:01.03 +41:23:26.6
00:44:50.41 +41:06:08.0
00:32:14.76 +43:02:06.8
00:32:58.65 +43:15:23.0
01:02:24.96 +47:26:32.9
00:43:47.17 +44:05:58.5
01:09:27.78 +42:40:17.6
00:31:22.40 +43:13:28.5
00:29:58.05 +41:56:50.4
00:29:26.96 +42:33:03.3
00:33:45.26 +46:31:47.2
00:51:14.82 +41:02:16.8
00:45:09.49 +48:17:57.1
00:33:58.45 +42:07:29.3
00:40:42.06 +48:34:27.0
00:41:47.58 +42:40:34.2
00:38:31.88 +41:33:57.7
00:46:54.07 +49:11:17.1
00:36:36.73 +46:12:55.9
00:30:15.39 +42:20:16.9
00:37:58.47 +42:40:08.9
00:49:53.72 +41:14:09.2
00:41:37.03 +41:40:20.0
00:34:52.33 +43:04:54.3
00:37:19.26 +45:51:17.0
00:27:43.16 +48:12:16.1
00:36:55.07 +42:20:24.3
00:32:07.96 +43:10:49.6
00:30:09.99 +42:25:39.4
00:36:22.72 +44:29:44.7
00:40:12.14 +46:51:11.0
00:33:48.89 +43:21:36.8
00:35:41.22 +45:20:46.4
00:31:56.09 +42:33:26.3
00:31:35.16 +41:47:32.7
00:38:58.18 +43:00:35.8
00:40:24.37 +44:01:18.8
00:35:10.32 +45:16:12.0
00:42:01.53 +42:36:59.2
00:48:43.63 +50:52:13.4
00:29:41.18 +44:27:34.1
00:37:32.75 +42:53:15.8
00:31:45.08 +45:04:33.0
00:31:41.15 +46:40:05.1
00:47:50.79 +50:26:10.8
00:37:13.63 +44:16:56.6
00:32:39.63 +44:55:13.9
00:34:08.08 +44:36:16.1
00:38:38.51 +43:48:31.3
00:33:43.43 +46:08:52.8
00:39:21.80 +43:26:05.0
00:31:38.64 +43:08:45.1
00:35:07.66 +44:27:31.7
00:42:44.69 +49:22:32.1
00:29:35.36 +48:43:49.5
00:41:50.00 +50:22:44.0
00:35:37.92 +50:50:42.2
00:28:04.77 +48:42:28.0
00:27:47.01 +48:44:55.4
00:39:27.37 +49:30:14.0
00:40:07.46 +50:58:10.9
00:28:10.52 +50:28:13.3
00:40:25.51 +50:06:20.4
00:27:37.26 +46:39:48.3
00:37:13.26 +49:18:30.1
00:34:29.11 +49:44:40.1
00:40:02.38 +48:45:55.9
00:29:10.89 +50:35:55.5
00:40:22.63 +48:24:40.9
00:40:47.98 +50:22:54.8
00:39:44.84 +48:49:09.3
00:30:43.02 +50:40:39.6
00:41:56.98 +50:23:36.6
00:27:32.70 +47:03:25.6
00:31:52.49 +46:21:57.7
00:28:25.81 +46:51:48.6
00:33:42.49 +47:24:29.0
00:34:42.15 +50:28:57.4
00:27:48.06 +50:07:21.0
00:36:47.71 +50:42:53.9
00:31:47.45 +47:44:57.0
00:27:51.93 +46:50:39.7
00:33:00.95 +44:43:33.1
00:25:56.30 +50:25:36.6
00:32:36.67 +50:35:50.6
00:32:52.46 +47:20:32.6
00:36:54.48 +41:38:02.8
00:34:00.37 +47:26:14.4
00:33:23.87 +47:46:20.3
00:34:15.21 +45:44:27.2
00:27:06.72 +48:44:44.8
00:30:11.27 +47:42:51.6
00:33:30.94 +50:15:17.7
00:27:22.09 +50:06:14.5
00:34:06.84 +50:18:15.7
00:29:57.12 +50:51:20.4
00:26:39.99 +50:38:49.0
00:28:26.73 +47:32:06.4
00:32:50.24 +48:02:08.2
00:32:55.26 +50:52:16.6
00:33:11.55 +46:20:28.4
00:26:08.30 +50:36:53.2
00:31:26.81 +49:04:41.2
00:32:11.73 +50:25:33.3
00:40:02.87 +49:44:40.7
00:27:11.90 +50:08:47.8
00:31:49.76 +49:28:28.9
00:31:45.63 +45:04:58.0
00:42:16.59 +50:56:56.4
00:26:00.85 +49:45:49.8
00:36:15.62 +50:44:15.3
00:46:23.83 +50:54:06.0
00:40:56.78 +48:54:08.4
00:33:15.77 +49:37:33.7
00:32:21.55 +48:47:50.3
00:26:52.85 +50:27:01.0
00:34:21.95 +48:11:20.7
00:32:46.50 +50:19:34.2
00:32:11.08 +50:39:26.7
00:28:11.47 +50:09:06.6
00:27:46.97 +47:26:24.2
00:31:34.11 +50:08:03.2
00:30:19.59 +41:10:31.5
00:29:39.45 +50:03:41.8
00:31:05.24 +50:41:52.8
00:44:15.48 +50:16:51.3
00:44:01.83 +50:08:46.5
00:47:43.48 +49:58:08.9
00:29:39.05 +50:11:50.6
00:34:30.33 +50:35:31.2
00:38:29.50 +49:12:54.5
00:29:53.31 +48:07:15.7
00:28:47.26 +48:40:22.0
00:31:06.74 +48:27:58.3
00:31:34.55 +50:52:17.7
00:39:40.82 +49:10:20.1
00:31:10.55 +50:45:01.0
00:25:16.94 +50:35:20.6
00:28:10.60 +50:15:18.0
00:29:11.46 +47:45:53.1
00:33:16.34 +50:44:11.8
00:49:44.43 +41:02:37.4
00:30:07.34 +50:12:32.0
00:30:08.25 +49:12:19.3
00:29:53.44 +50:11:02.4
00:29:38.30 +42:09:08.4
00:34:40.69 +50:22:02.5
00:25:55.21 +49:48:43.2
00:28:45.96 +49:15:40.7
00:39:53.15 +50:41:16.4
00:43:01.54 +51:05:22.7
00:36:16.28 +49:53:12.7
00:32:35.02 +50:01:53.6
00:28:48.90 +43:56:36.2
00:27:29.41 +48:06:06.0
00:28:37.06 +46:18:09.9
00:46:52.35 +49:51:39.6
00:29:25.74 +49:41:21.6
00:27:06.50 +49:21:19.4
00:27:59.35 +50:27:49.0
00:42:50.51 +44:36:28.4
00:30:45.47 +45:18:50.6
00:36:25.68 +45:37:21.6
00:27:08.87 +49:17:55.6
00:26:33.82 +49:33:37.5
00:26:03.00 +50:33:43.8
00:51:20.35 +44:10:03.3
00:38:19.68 +50:40:00.1
00:32:45.06 +49:39:07.0
00:42:09.80 +50:45:46.9
00:30:23.89 +50:09:25.7
00:42:38.98 +46:09:02.8
00:33:43.39 +49:45:58.5
00:42:03.89 +50:21:14.9
00:32:30.81 +50:25:45.1
00:31:01.26 +47:46:46.6
00:29:14.34 +50:34:30.0
00:34:06.37 +43:14:12.9
00:29:48.22 +44:49:04.6
00:43:04.15 +51:04:00.3
00:30:17.47 +50:24:00.2
00:30:53.38 +47:32:54.7
00:26:55.34 +50:42:07.9
00:27:10.48 +49:24:48.3
00:26:22.18 +50:49:08.2
00:40:39.37 +50:04:30.0
00:38:24.31 +50:36:29.7
00:35:25.45 +50:14:35.3
00:28:47.38 +50:31:19.7
00:26:39.13 +50:15:24.8
00:32:49.84 +49:47:49.1
00:36:38.47 +42:10:48.9
00:39:19.76 +49:52:02.7
00:33:54.83 +50:30:03.4
00:30:47.73 +49:36:54.7
00:35:57.52 +44:26:05.3
00:38:45.82 +43:18:53.7
00:25:46.69 +49:53:38.0
00:31:56.93 +49:43:55.5
00:34:22.56 +49:51:07.5
00:26:47.68 +48:10:38.5
00:26:48.36 +48:10:42.3
00:32:17.11 +50:32:02.5
00:30:17.55 +44:55:50.5
00:27:52.04 +49:20:06.7
00:27:31.27 +47:36:58.9
00:33:57.83 +49:37:29.4
00:26:11.72 +50:49:43.5
00:32:27.85 +44:48:22.3
00:28:33.50 +44:52:49.4
00:33:24.86 +41:45:46.1
00:32:39.56 +50:18:05.6
00:29:11.93 +45:39:08.5
00:27:32.67 +49:57:23.8
00:27:43.85 +49:51:46.5
00:34:24.44 +50:39:44.8
00:27:06.77 +50:39:40.1
00:32:17.53 +50:32:04.4
00:29:26.36 +49:15:10.3
00:26:22.26 +49:05:47.5
01:55:41.06 +50:00:11.6
00:33:53.67 +50:00:13.5
00:42:59.68 +50:33:07.4
00:34:43.74 +43:16:57.3
00:30:06.90 +49:21:47.8
00:27:17.58 +48:55:28.3
00:29:40.13 +48:41:42.0
00:27:31.22 +46:55:30.7
00:32:44.96 +47:06:11.4
00:26:35.88 +48:52:42.5
00:28:50.50 +50:45:50.7
00:34:32.15 +43:30:48.6
00:27:55.45 +50:17:57.2
00:36:52.19 +49:27:44.5
00:27:26.86 +48:32:01.5
00:27:44.21 +50:49:28.8
00:32:55.99 +47:12:34.8
00:26:03.54 +49:35:56.5
00:40:15.10 +50:56:11.3
00:30:24.08 +41:20:21.0
00:28:14.64 +48:43:14.6
00:33:54.10 +47:12:58.0
00:25:35.00 +50:09:14.2
01:16:04.64 +50:11:40.0
01:14:22.06 +49:58:28.9
00:30:08.26 +49:34:49.0
01:20:54.65 +49:35:51.8
01:28:03.50 +49:29:53.6
01:06:04.74 +49:51:20.0
01:16:57.43 +49:34:43.7
01:23:44.50 +49:24:07.3
01:00:21.25 +48:54:15.3
00:29:25.84 +48:36:05.5
00:56:40.47 +48:44:11.4
01:00:04.24 +48:40:23.8
00:57:04.39 +48:42:09.0
00:47:53.15 +48:30:44.7
01:37:29.69 +47:55:39.9
00:49:08.09 +48:12:50.7
01:31:04.14 +47:34:41.3
01:17:29.78 +47:41:12.0
01:26:55.54 +47:24:02.8
01:23:46.35 +47:16:25.4
01:06:23.29 +47:20:01.6
01:14:22.24 +47:04:47.6
01:31:54.80 +46:49:07.2
00:49:14.16 +46:59:32.7
01:22:04.52 +46:06:40.4
01:23:44.46 +45:52:03.1
01:07:26.54 +45:36:35.6
01:24:25.24 +45:36:20.1
00:38:53.25 +45:33:49.7
########### Completed And-02-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 ####
00:29:32.62 +49:25:24.8
00:44:52.14 +46:14:18.9
00:34:34.69 +42:09:25.3
00:54:37.50 +49:28:21.1
00:38:39.17 +43:48:36.1
00:33:45.23 +42:24:49.0
00:35:55.68 +42:23:43.1
00:40:58.52 +41:43:55.5
00:42:32.09 +40:57:18.8
00:39:19.95 +41:55:34.6
00:46:22.18 +50:04:38.5
00:52:57.44 +50:46:08.6
00:33:22.70 +49:51:24.6
00:34:27.80 +49:19:12.3
00:40:15.19 +50:49:23.2
00:42:38.80 +49:34:51.5
00:28:11.05 +50:28:08.9
00:33:55.33 +48:39:10.4
00:35:43.70 +41:45:08.4
00:28:05.04 +49:10:14.5
00:31:28.44 +49:04:22.2
00:36:27.59 +50:58:06.8
00:25:16.24 +50:31:57.6
00:46:51.43 +42:18:06.4
00:32:50.53 +49:19:44.5
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00:55:15.09 +49:39:22.0
00:36:48.66 +50:42:52.3
00:31:44.18 +50:02:56.2
01:31:58.34 +45:46:20.7
01:16:19.81 +47:27:31.0
01:15:42.26 +46:12:18.4
01:25:48.53 +46:24:13.0
01:14:04.52 +47:52:07.5
01:10:12.93 +49:10:15.4
00:58:20.83 +49:25:06.4
00:45:56.25 +50:23:15.7
01:26:27.60 +49:53:58.1
01:33:35.62 +46:31:13.7
00:40:54.80 +43:18:07.5
00:41:27.98 +44:06:28.9
01:00:20.71 +41:01:19.8
00:45:14.07 +41:03:01.6
00:29:49.36 +41:44:42.3
00:44:05.02 +42:19:57.0
01:29:26.69 +46:27:24.0
01:28:47.66 +44:16:39.2
00:56:54.71 +41:31:41.7
00:46:26.17 +45:54:34.7
00:32:49.44 +41:33:51.5
00:42:36.20 +44:15:33.5
01:51:23.52 +49:56:14.5
00:39:05.16 +40:55:41.8
00:30:50.10 +41:16:32.5
00:40:06.38 +42:22:42.1
00:32:34.15 +48:41:56.2
00:42:10.50 +41:26:20.5
00:39:18.12 +49:31:27.4
00:46:32.24 +41:51:49.3
00:31:15.32 +44:21:00.0
00:31:08.32 +42:49:07.5
00:42:58.20 +40:58:58.5
00:29:18.89 +46:12:00.8
00:38:14.08 +42:16:52.0
01:21:11.80 +48:29:08.2
00:40:19.55 +43:04:59.3
00:30:51.74 +41:44:46.9
00:43:44.55 +41:04:55.1
00:36:25.74 +42:34:30.4
00:49:17.74 +42:47:31.3
00:40:33.46 +44:20:49.8
00:30:55.16 +50:04:24.3
00:40:14.45 +44:46:47.0
00:42:21.35 +45:04:14.7
00:39:07.27 +48:10:19.6
01:19:23.91 +48:26:38.1
00:36:25.84 +41:03:26.3
00:31:05.63 +46:50:59.2
00:45:08.14 +46:22:02.1
00:45:46.38 +42:25:21.5
00:45:32.07 +42:27:42.3
00:42:59.97 +41:05:53.6
00:35:36.91 +43:02:35.6
00:38:24.78 +44:16:41.4
00:37:27.73 +42:03:43.4
00:33:09.14 +42:48:18.3
00:36:54.15 +48:50:38.7
00:38:17.33 +43:36:12.0
00:35:46.84 +41:39:44.1
00:35:38.15 +41:02:02.2
00:54:44.06 +41:23:44.1
00:38:32.84 +43:35:18.0
00:40:04.02 +42:13:37.6
00:49:57.43 +45:10:25.3
00:42:19.61 +42:25:25.9
00:35:02.82 +42:35:09.7
00:33:09.09 +42:48:22.6
00:36:49.40 +44:35:15.5
00:37:34.52 +44:27:48.1
00:41:27.25 +42:12:52.2
00:32:54.83 +41:50:09.4
00:32:55.07 +40:52:22.6
00:35:44.15 +41:15:09.3
00:40:38.56 +43:06:25.1
00:43:11.12 +41:36:14.9
00:33:27.98 +44:19:03.1
01:10:43.33 +43:20:57.2
00:45:35.47 +43:34:46.5
00:44:52.33 +41:25:03.3
00:37:48.84 +43:51:08.4
00:35:00.04 +42:13:42.7
00:36:28.24 +44:27:45.7
00:40:45.58 +42:16:48.8
00:29:04.68 +46:31:28.9
00:46:37.44 +41:08:56.1
00:44:53.46 +49:53:06.5
00:43:00.26 +41:28:54.6
00:31:24.11 +44:25:24.4
00:42:30.39 +44:32:12.6
00:41:21.83 +46:23:45.3
00:39:41.74 +41:26:54.8
00:32:54.29 +47:07:43.0
00:27:31.57 +48:49:15.5
00:42:24.39 +43:09:57.8
00:55:13.37 +46:39:01.7
00:47:20.19 +43:53:19.0
00:33:35.66 +45:30:31.1
01:11:14.09 +50:23:29.3
00:35:45.77 +49:23:12.7
00:44:08.79 +42:27:38.3
00:40:42.40 +48:48:37.5
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00:39:40.82 +49:10:20.1
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00:25:16.94 +50:35:20.6
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00:30:07.34 +50:12:32.0
00:30:08.25 +49:12:19.3
00:29:53.44 +50:11:02.4
00:29:38.30 +42:09:08.4
00:34:40.69 +50:22:02.5
00:25:55.21 +49:48:43.2
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00:32:35.02 +50:01:53.6
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00:27:29.41 +48:06:06.0
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00:46:52.35 +49:51:39.6
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00:30:45.47 +45:18:50.6
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00:26:03.00 +50:33:43.8
00:51:20.35 +44:10:03.3
00:38:19.68 +50:40:00.1
00:32:45.06 +49:39:07.0
00:42:09.80 +50:45:46.9
00:30:23.89 +50:09:25.7
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00:33:43.39 +49:45:58.5
00:42:03.89 +50:21:14.9
00:32:30.81 +50:25:45.1
00:31:01.26 +47:46:46.6
00:29:14.34 +50:34:30.0
00:34:06.37 +43:14:12.9
00:29:48.22 +44:49:04.6
00:43:04.15 +51:04:00.3
00:30:17.47 +50:24:00.2
00:30:53.38 +47:32:54.7
00:26:55.34 +50:42:07.9
00:27:10.48 +49:24:48.3
00:26:22.18 +50:49:08.2
00:40:39.37 +50:04:30.0
00:38:24.31 +50:36:29.7
00:35:25.45 +50:14:35.3
00:28:47.38 +50:31:19.7
00:26:39.13 +50:15:24.8
00:32:49.84 +49:47:49.1
00:36:38.47 +42:10:48.9
00:39:19.76 +49:52:02.7
00:33:54.83 +50:30:03.4
00:30:47.73 +49:36:54.7
00:35:57.52 +44:26:05.3
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00:25:46.69 +49:53:38.0
00:31:56.93 +49:43:55.5
00:34:22.56 +49:51:07.5
00:26:47.68 +48:10:38.5
00:26:48.36 +48:10:42.3
00:32:17.11 +50:32:02.5
00:30:17.55 +44:55:50.5
00:27:52.04 +49:20:06.7
00:27:31.27 +47:36:58.9
00:33:57.83 +49:37:29.4
00:26:11.72 +50:49:43.5
00:32:27.85 +44:48:22.3
00:28:33.50 +44:52:49.4
00:33:24.86 +41:45:46.1
00:32:39.56 +50:18:05.6
00:29:11.93 +45:39:08.5
00:27:32.67 +49:57:23.8
00:27:43.85 +49:51:46.5
00:34:24.44 +50:39:44.8
00:27:06.77 +50:39:40.1
00:32:17.53 +50:32:04.4
00:29:26.36 +49:15:10.3
00:26:22.26 +49:05:47.5
01:55:41.06 +50:00:11.6
00:33:53.67 +50:00:13.5
00:42:59.68 +50:33:07.4
00:34:43.74 +43:16:57.3
00:30:06.90 +49:21:47.8
00:27:17.58 +48:55:28.3
00:29:40.13 +48:41:42.0
00:27:31.22 +46:55:30.7
00:32:44.96 +47:06:11.4
00:26:35.88 +48:52:42.5
00:28:50.50 +50:45:50.7
00:34:32.15 +43:30:48.6
00:27:55.45 +50:17:57.2
00:36:52.19 +49:27:44.5
00:27:26.86 +48:32:01.5
00:27:44.21 +50:49:28.8
00:32:55.99 +47:12:34.8
00:26:03.54 +49:35:56.5
00:40:15.10 +50:56:11.3
00:30:24.08 +41:20:21.0
00:28:14.64 +48:43:14.6
00:33:54.10 +47:12:58.0
00:25:35.00 +50:09:14.2
00:30:08.26 +49:34:49.0
00:38:56.24 +50:58:31.5
00:54:54.46 +41:10:28.6
01:20:28.68 +43:52:02.2
01:28:03.50 +49:29:53.6
01:16:04.64 +50:11:40.0
01:23:44.50 +49:24:07.3
01:17:55.72 +50:24:13.4
00:47:53.15 +48:30:44.7
01:10:12.11 +50:22:50.0
01:00:04.24 +48:40:23.8
01:31:54.80 +46:49:07.2
00:29:25.84 +48:36:05.5
00:49:14.16 +46:59:32.7
01:16:57.43 +49:34:43.7
01:17:29.78 +47:41:12.0
01:23:46.35 +47:16:25.4
00:56:40.47 +48:44:11.4
01:12:32.83 +50:51:24.3
01:20:54.65 +49:35:51.8
01:11:45.37 +43:16:18.1
00:49:08.09 +48:12:50.7
00:32:18.61 +50:27:38.4
00:38:53.25 +45:33:49.7
00:35:44.05 +50:33:08.7
00:57:28.45 +42:47:54.3
01:24:25.24 +45:36:20.1
01:06:04.74 +49:51:20.0
00:43:46.56 +51:02:35.7
01:14:22.24 +47:04:47.6
00:51:23.98 +49:09:52.9
01:37:29.69 +47:55:39.9
01:26:55.54 +47:24:02.8
01:36:40.37 +42:51:19.4
01:22:04.52 +46:06:40.4
01:31:04.14 +47:34:41.3
00:54:27.34 +43:55:38.0
01:00:48.10 +50:23:41.6
01:35:12.12 +46:33:47.6
01:06:23.29 +47:20:01.6
01:07:26.54 +45:36:35.6
01:21:37.14 +43:32:51.2
01:23:44.46 +45:52:03.1
01:00:21.25 +48:54:15.3
01:14:22.06 +49:58:28.9
00:57:04.39 +48:42:09.0
###################################################################################
00:29:32.62 +49:25:24.8 -- not an asteroid (will add it to exclusion list)
00:44:52.14 +46:14:18.9 -- not an asteroid (will add it to exclusion list)
00:34:34.69 +42:09:25.3 -- not an asteroid (will add it to exclusion list)
00:54:37.50 +49:28:21.1 -- not an asteroid (will add it to exclusion list)
00:38:39.17 +43:48:36.1 -- not an asteroid (will add it to exclusion list)
00:33:45.23 +42:24:49.0 -- not an asteroid (will add it to exclusion list)
00:35:55.68 +42:23:43.1 -- not an asteroid (will add it to exclusion list)
00:40:58.52 +41:43:55.5 -- not an asteroid (will add it to exclusion list)
00:42:32.09 +40:57:18.8 -- not an asteroid (will add it to exclusion list)
00:39:19.95 +41:55:34.6 -- not an asteroid (will add it to exclusion list)
00:46:22.18 +50:04:38.5 -- not an asteroid (will add it to exclusion list)
00:52:57.44 +50:46:08.6 -- not an asteroid (will add it to exclusion list)
00:33:22.70 +49:51:24.6 -- not an asteroid (will add it to exclusion list)
00:34:27.80 +49:19:12.3 -- not an asteroid (will add it to exclusion list)
00:40:15.19 +50:49:23.2 -- not an asteroid (will add it to exclusion list)
00:42:38.80 +49:34:51.5 -- not an asteroid (will add it to exclusion list)
00:28:11.05 +50:28:08.9 -- not an asteroid (will add it to exclusion list)
00:33:55.33 +48:39:10.4 -- not an asteroid (will add it to exclusion list)
00:35:43.70 +41:45:08.4 -- not an asteroid (will add it to exclusion list)
00:28:05.04 +49:10:14.5 -- not an asteroid (will add it to exclusion list)
00:31:28.44 +49:04:22.2 -- not an asteroid (will add it to exclusion list)
00:36:27.59 +50:58:06.8 -- not an asteroid (will add it to exclusion list)
00:25:16.24 +50:31:57.6 -- not an asteroid (will add it to exclusion list)
00:46:51.43 +42:18:06.4 -- not an asteroid (will add it to exclusion list)
00:32:50.53 +49:19:44.5 -- not an asteroid (will add it to exclusion list)
00:26:49.68 +50:46:16.7 -- not an asteroid (will add it to exclusion list)
00:55:15.09 +49:39:22.0 -- not an asteroid (will add it to exclusion list)
00:36:48.66 +50:42:52.3 -- not an asteroid (will add it to exclusion list)
00:31:44.18 +50:02:56.2 -- not an asteroid (will add it to exclusion list)
01:31:58.34 +45:46:20.7 -- not an asteroid (will add it to exclusion list)
01:16:19.81 +47:27:31.0 -- not an asteroid (will add it to exclusion list)
01:15:42.26 +46:12:18.4 -- not an asteroid (will add it to exclusion list)
01:25:48.53 +46:24:13.0 -- not an asteroid (will add it to exclusion list)
01:14:04.52 +47:52:07.5 -- not an asteroid (will add it to exclusion list)
01:10:12.93 +49:10:15.4 -- not an asteroid (will add it to exclusion list)
00:58:20.83 +49:25:06.4 -- not an asteroid (will add it to exclusion list)
00:45:56.25 +50:23:15.7 -- not an asteroid (will add it to exclusion list)
01:26:27.60 +49:53:58.1 -- not an asteroid (will add it to exclusion list)
01:33:35.62 +46:31:13.7 -- not an asteroid (will add it to exclusion list)
00:40:54.80 +43:18:07.5 -- not an asteroid (will add it to exclusion list)
00:41:27.98 +44:06:28.9 -- not an asteroid (will add it to exclusion list)
01:00:20.71 +41:01:19.8 -- not an asteroid (will add it to exclusion list)
00:45:14.07 +41:03:01.6 -- not an asteroid (will add it to exclusion list)
00:29:49.36 +41:44:42.3 -- not an asteroid (will add it to exclusion list)
00:44:05.02 +42:19:57.0 -- not an asteroid (will add it to exclusion list)
01:29:26.69 +46:27:24.0 -- not an asteroid (will add it to exclusion list)
01:28:47.66 +44:16:39.2 -- not an asteroid (will add it to exclusion list)
00:56:54.71 +41:31:41.7 -- not an asteroid (will add it to exclusion list)
00:46:26.17 +45:54:34.7 -- not an asteroid (will add it to exclusion list)
00:32:49.44 +41:33:51.5 -- not an asteroid (will add it to exclusion list)
00:42:36.20 +44:15:33.5 -- not an asteroid (will add it to exclusion list)
01:51:23.52 +49:56:14.5 -- not an asteroid (will add it to exclusion list)
00:39:05.16 +40:55:41.8 -- not an asteroid (will add it to exclusion list)
00:30:50.10 +41:16:32.5 -- not an asteroid (will add it to exclusion list)
00:40:06.38 +42:22:42.1 -- not an asteroid (will add it to exclusion list)
00:32:34.15 +48:41:56.2 -- not an asteroid (will add it to exclusion list)
00:42:10.50 +41:26:20.5 -- not an asteroid (will add it to exclusion list)
00:39:18.12 +49:31:27.4 -- not an asteroid (will add it to exclusion list)
00:46:32.24 +41:51:49.3 -- not an asteroid (will add it to exclusion list)
00:31:15.32 +44:21:00.0 -- not an asteroid (will add it to exclusion list)
00:31:08.32 +42:49:07.5 -- not an asteroid (will add it to exclusion list)
00:42:58.20 +40:58:58.5 -- not an asteroid (will add it to exclusion list)
00:29:18.89 +46:12:00.8 -- not an asteroid (will add it to exclusion list)
00:38:14.08 +42:16:52.0 -- not an asteroid (will add it to exclusion list)
01:21:11.80 +48:29:08.2 -- not an asteroid (will add it to exclusion list)
00:40:19.55 +43:04:59.3 -- not an asteroid (will add it to exclusion list)
00:30:51.74 +41:44:46.9 -- not an asteroid (will add it to exclusion list)
00:43:44.55 +41:04:55.1 -- not an asteroid (will add it to exclusion list)
00:36:25.74 +42:34:30.4 -- not an asteroid (will add it to exclusion list)
00:49:17.74 +42:47:31.3 -- not an asteroid (will add it to exclusion list)
00:40:33.46 +44:20:49.8 -- not an asteroid (will add it to exclusion list)
00:30:55.16 +50:04:24.3 -- not an asteroid (will add it to exclusion list)
00:40:14.45 +44:46:47.0 -- not an asteroid (will add it to exclusion list)
00:42:21.35 +45:04:14.7 -- not an asteroid (will add it to exclusion list)
00:39:07.27 +48:10:19.6 -- not an asteroid (will add it to exclusion list)
01:19:23.91 +48:26:38.1 -- not an asteroid (will add it to exclusion list)
00:36:25.84 +41:03:26.3 -- not an asteroid (will add it to exclusion list)
00:31:05.63 +46:50:59.2 -- not an asteroid (will add it to exclusion list)
00:45:08.14 +46:22:02.1 -- not an asteroid (will add it to exclusion list)
00:45:46.38 +42:25:21.5 -- not an asteroid (will add it to exclusion list)
00:45:32.07 +42:27:42.3 -- not an asteroid (will add it to exclusion list)
00:42:59.97 +41:05:53.6 -- not an asteroid (will add it to exclusion list)
00:35:36.91 +43:02:35.6 -- not an asteroid (will add it to exclusion list)
00:38:24.78 +44:16:41.4 -- not an asteroid (will add it to exclusion list)
00:37:27.73 +42:03:43.4 -- not an asteroid (will add it to exclusion list)
00:33:09.14 +42:48:18.3 -- not an asteroid (will add it to exclusion list)
00:36:54.15 +48:50:38.7 -- not an asteroid (will add it to exclusion list)
00:38:17.33 +43:36:12.0 -- not an asteroid (will add it to exclusion list)
00:35:46.84 +41:39:44.1 -- not an asteroid (will add it to exclusion list)
00:35:38.15 +41:02:02.2 -- not an asteroid (will add it to exclusion list)
00:54:44.06 +41:23:44.1 -- not an asteroid (will add it to exclusion list)
00:38:32.84 +43:35:18.0 -- not an asteroid (will add it to exclusion list)
00:40:04.02 +42:13:37.6 -- not an asteroid (will add it to exclusion list)
00:49:57.43 +45:10:25.3 -- not an asteroid (will add it to exclusion list)
00:42:19.61 +42:25:25.9 -- not an asteroid (will add it to exclusion list)
00:35:02.82 +42:35:09.7 -- not an asteroid (will add it to exclusion list)
00:33:09.09 +42:48:22.6 -- not an asteroid (will add it to exclusion list)
00:36:49.40 +44:35:15.5 -- not an asteroid (will add it to exclusion list)
00:37:34.52 +44:27:48.1 -- not an asteroid (will add it to exclusion list)
00:41:27.25 +42:12:52.2 -- not an asteroid (will add it to exclusion list)
00:32:54.83 +41:50:09.4 -- not an asteroid (will add it to exclusion list)
00:32:55.07 +40:52:22.6 -- not an asteroid (will add it to exclusion list)
00:35:44.15 +41:15:09.3 -- not an asteroid (will add it to exclusion list)
00:40:38.56 +43:06:25.1 -- not an asteroid (will add it to exclusion list)
00:43:11.12 +41:36:14.9 -- not an asteroid (will add it to exclusion list)
00:33:27.98 +44:19:03.1 -- not an asteroid (will add it to exclusion list)
01:10:43.33 +43:20:57.2 -- not an asteroid (will add it to exclusion list)
00:45:35.47 +43:34:46.5 -- not an asteroid (will add it to exclusion list)
00:44:52.33 +41:25:03.3 -- not an asteroid (will add it to exclusion list)
00:37:48.84 +43:51:08.4 -- not an asteroid (will add it to exclusion list)
00:35:00.04 +42:13:42.7 -- not an asteroid (will add it to exclusion list)
00:36:28.24 +44:27:45.7 -- not an asteroid (will add it to exclusion list)
00:40:45.58 +42:16:48.8 -- not an asteroid (will add it to exclusion list)
00:29:04.68 +46:31:28.9 -- not an asteroid (will add it to exclusion list)
00:46:37.44 +41:08:56.1 -- not an asteroid (will add it to exclusion list)
00:44:53.46 +49:53:06.5 -- not an asteroid (will add it to exclusion list)
00:43:00.26 +41:28:54.6 -- not an asteroid (will add it to exclusion list)
00:31:24.11 +44:25:24.4 -- not an asteroid (will add it to exclusion list)
00:42:30.39 +44:32:12.6 -- not an asteroid (will add it to exclusion list)
00:41:21.83 +46:23:45.3 -- not an asteroid (will add it to exclusion list)
00:39:41.74 +41:26:54.8 -- not an asteroid (will add it to exclusion list)
00:32:54.29 +47:07:43.0 -- not an asteroid (will add it to exclusion list)
00:27:31.57 +48:49:15.5 -- not an asteroid (will add it to exclusion list)
00:42:24.39 +43:09:57.8 -- not an asteroid (will add it to exclusion list)
00:55:13.37 +46:39:01.7 -- not an asteroid (will add it to exclusion list)
00:47:20.19 +43:53:19.0 -- not an asteroid (will add it to exclusion list)
00:33:35.66 +45:30:31.1 -- not an asteroid (will add it to exclusion list)
01:11:14.09 +50:23:29.3 -- not an asteroid (will add it to exclusion list)
00:35:45.77 +49:23:12.7 -- not an asteroid (will add it to exclusion list)
00:44:08.79 +42:27:38.3 -- not an asteroid (will add it to exclusion list)
00:40:42.40 +48:48:37.5 -- not an asteroid (will add it to exclusion list)
00:33:28.11 +42:03:50.7 -- not an asteroid (will add it to exclusion list)
00:38:45.74 +43:49:49.7 -- not an asteroid (will add it to exclusion list)
00:42:52.87 +43:18:59.8 -- not an asteroid (will add it to exclusion list)
00:40:46.85 +50:18:46.7 -- not an asteroid (will add it to exclusion list)
00:39:18.67 +48:30:25.9 -- not an asteroid (will add it to exclusion list)
00:38:48.42 +46:30:21.2 -- not an asteroid (will add it to exclusion list)
00:30:50.61 +43:43:00.9 -- not an asteroid (will add it to exclusion list)
00:36:22.78 +50:38:17.7 -- not an asteroid (will add it to exclusion list)
01:07:07.67 +43:02:44.6 -- not an asteroid (will add it to exclusion list)
00:51:35.56 +41:37:04.6 -- not an asteroid (will add it to exclusion list)
00:36:34.59 +49:09:03.9 -- not an asteroid (will add it to exclusion list)
00:27:53.38 +46:08:08.5 -- not an asteroid (will add it to exclusion list)
00:37:30.07 +45:50:30.3 -- not an asteroid (will add it to exclusion list)
00:55:48.81 +44:10:48.4 -- not an asteroid (will add it to exclusion list)
00:29:05.57 +45:41:25.8 -- not an asteroid (will add it to exclusion list)
00:35:25.34 +49:55:43.8 -- not an asteroid (will add it to exclusion list)
00:36:29.53 +49:32:09.7 -- not an asteroid (will add it to exclusion list)
00:40:55.67 +40:57:43.4 -- not an asteroid (will add it to exclusion list)
00:41:18.74 +44:10:21.0 -- not an asteroid (will add it to exclusion list)
00:34:28.88 +42:30:06.4 -- not an asteroid (will add it to exclusion list)
00:51:55.88 +51:02:22.0 -- not an asteroid (will add it to exclusion list)
00:33:59.04 +50:30:22.6 -- not an asteroid (will add it to exclusion list)
00:43:25.55 +41:24:23.1 -- not an asteroid (will add it to exclusion list)
00:28:39.06 +46:42:07.2 -- not an asteroid (will add it to exclusion list)
00:46:38.86 +42:57:47.0 -- not an asteroid (will add it to exclusion list)
00:33:55.78 +46:08:48.1 -- not an asteroid (will add it to exclusion list)
00:36:00.05 +46:04:24.3 -- not an asteroid (will add it to exclusion list)
00:38:51.55 +43:44:31.9 -- not an asteroid (will add it to exclusion list)
00:45:30.88 +40:58:40.2 -- not an asteroid (will add it to exclusion list)
00:42:11.80 +48:53:19.9 -- not an asteroid (will add it to exclusion list)
00:30:44.42 +47:48:53.3 -- not an asteroid (will add it to exclusion list)
00:39:02.12 +49:30:32.7 -- not an asteroid (will add it to exclusion list)
00:34:35.69 +47:34:42.4 -- not an asteroid (will add it to exclusion list)
00:49:36.89 +41:29:06.4 -- not an asteroid (will add it to exclusion list)
00:32:50.08 +42:34:54.4 -- not an asteroid (will add it to exclusion list)
00:39:25.42 +47:25:28.8 -- not an asteroid (will add it to exclusion list)
00:34:42.75 +43:33:40.6 -- not an asteroid (will add it to exclusion list)
00:37:33.86 +41:55:06.5 -- not an asteroid (will add it to exclusion list)
00:32:04.48 +43:46:41.9 -- not an asteroid (will add it to exclusion list)
00:36:05.33 +44:20:32.8 -- not an asteroid (will add it to exclusion list)
00:52:35.41 +44:54:12.9 -- not an asteroid (will add it to exclusion list)
00:35:45.81 +42:25:30.9 -- not an asteroid (will add it to exclusion list)
00:30:30.05 +44:28:06.2 -- not an asteroid (will add it to exclusion list)
00:38:46.51 +46:52:37.6 -- not an asteroid (will add it to exclusion list)
01:03:40.80 +48:10:46.9 -- not an asteroid (will add it to exclusion list)
00:47:55.32 +49:51:36.5 -- not an asteroid (will add it to exclusion list)
00:40:03.46 +41:19:01.0 -- not an asteroid (will add it to exclusion list)
00:33:39.87 +44:07:45.0 -- not an asteroid (will add it to exclusion list)
00:46:17.98 +50:52:33.5 -- not an asteroid (will add it to exclusion list)
00:27:54.37 +49:29:44.4 -- not an asteroid (will add it to exclusion list)
00:36:36.31 +41:42:11.7 -- not an asteroid (will add it to exclusion list)
00:39:40.36 +42:36:07.8 -- not an asteroid (will add it to exclusion list)
00:34:59.13 +43:38:26.1 -- not an asteroid (will add it to exclusion list)
01:13:46.30 +46:34:07.8 -- not an asteroid (will add it to exclusion list)
00:37:41.55 +47:58:23.2 -- not an asteroid (will add it to exclusion list)
00:47:49.56 +48:00:39.9 -- not an asteroid (will add it to exclusion list)
00:37:40.43 +46:38:53.5 -- not an asteroid (will add it to exclusion list)
00:28:53.47 +44:15:58.5 -- not an asteroid (will add it to exclusion list)
01:05:51.98 +48:50:26.6 -- not an asteroid (will add it to exclusion list)
00:34:14.62 +42:15:49.1 -- not an asteroid (will add it to exclusion list)
00:36:01.03 +41:23:26.6 -- not an asteroid (will add it to exclusion list)
00:44:50.41 +41:06:08.0 -- not an asteroid (will add it to exclusion list)
00:32:14.76 +43:02:06.8 -- not an asteroid (will add it to exclusion list)
00:32:58.65 +43:15:23.0 -- not an asteroid (will add it to exclusion list)
01:02:24.96 +47:26:32.9 -- not an asteroid (will add it to exclusion list)
00:43:47.17 +44:05:58.5 -- not an asteroid (will add it to exclusion list)
01:09:27.78 +42:40:17.6 -- not an asteroid (will add it to exclusion list)
00:31:22.40 +43:13:28.5 -- not an asteroid (will add it to exclusion list)
00:29:58.05 +41:56:50.4 -- not an asteroid (will add it to exclusion list)
00:29:26.96 +42:33:03.3 -- not an asteroid (will add it to exclusion list)
00:33:45.26 +46:31:47.2 -- not an asteroid (will add it to exclusion list)
00:51:14.82 +41:02:16.8 -- not an asteroid (will add it to exclusion list)
00:45:09.49 +48:17:57.1 -- not an asteroid (will add it to exclusion list)
00:33:58.45 +42:07:29.3 -- not an asteroid (will add it to exclusion list)
00:40:42.06 +48:34:27.0 -- not an asteroid (will add it to exclusion list)
00:41:47.58 +42:40:34.2 -- not an asteroid (will add it to exclusion list)
00:38:31.88 +41:33:57.7 -- not an asteroid (will add it to exclusion list)
00:46:54.07 +49:11:17.1 -- not an asteroid (will add it to exclusion list)
00:36:36.73 +46:12:55.9 -- not an asteroid (will add it to exclusion list)
00:30:15.39 +42:20:16.9 -- not an asteroid (will add it to exclusion list)
00:37:58.47 +42:40:08.9 -- not an asteroid (will add it to exclusion list)
00:49:53.72 +41:14:09.2 -- not an asteroid (will add it to exclusion list)
00:41:37.03 +41:40:20.0 -- not an asteroid (will add it to exclusion list)
00:34:52.33 +43:04:54.3 -- not an asteroid (will add it to exclusion list)
00:37:19.26 +45:51:17.0 -- not an asteroid (will add it to exclusion list)
00:27:43.16 +48:12:16.1 -- not an asteroid (will add it to exclusion list)
00:36:55.07 +42:20:24.3 -- not an asteroid (will add it to exclusion list)
00:32:07.96 +43:10:49.6 -- not an asteroid (will add it to exclusion list)
00:30:09.99 +42:25:39.4 -- not an asteroid (will add it to exclusion list)
00:36:22.72 +44:29:44.7 -- not an asteroid (will add it to exclusion list)
00:40:12.14 +46:51:11.0 -- not an asteroid (will add it to exclusion list)
00:33:48.89 +43:21:36.8 -- not an asteroid (will add it to exclusion list)
00:35:41.22 +45:20:46.4 -- not an asteroid (will add it to exclusion list)
00:31:56.09 +42:33:26.3 -- not an asteroid (will add it to exclusion list)
00:31:35.16 +41:47:32.7 -- not an asteroid (will add it to exclusion list)
00:38:58.18 +43:00:35.8 -- not an asteroid (will add it to exclusion list)
00:40:24.37 +44:01:18.8 -- not an asteroid (will add it to exclusion list)
00:35:10.32 +45:16:12.0 -- not an asteroid (will add it to exclusion list)
00:42:01.53 +42:36:59.2 -- not an asteroid (will add it to exclusion list)
00:48:43.63 +50:52:13.4 -- not an asteroid (will add it to exclusion list)
00:29:41.18 +44:27:34.1 -- not an asteroid (will add it to exclusion list)
00:37:32.75 +42:53:15.8 -- not an asteroid (will add it to exclusion list)
00:31:45.08 +45:04:33.0 -- not an asteroid (will add it to exclusion list)
00:31:41.15 +46:40:05.1 -- not an asteroid (will add it to exclusion list)
00:47:50.79 +50:26:10.8 -- not an asteroid (will add it to exclusion list)
00:37:13.63 +44:16:56.6 -- not an asteroid (will add it to exclusion list)
00:32:39.63 +44:55:13.9 -- not an asteroid (will add it to exclusion list)
00:34:08.08 +44:36:16.1 -- not an asteroid (will add it to exclusion list)
00:38:38.51 +43:48:31.3 -- not an asteroid (will add it to exclusion list)
00:33:43.43 +46:08:52.8 -- not an asteroid (will add it to exclusion list)
00:39:21.80 +43:26:05.0 -- not an asteroid (will add it to exclusion list)
00:31:38.64 +43:08:45.1 -- not an asteroid (will add it to exclusion list)
00:35:07.66 +44:27:31.7 -- not an asteroid (will add it to exclusion list)
00:42:44.69 +49:22:32.1 -- not an asteroid (will add it to exclusion list)
00:29:35.36 +48:43:49.5 -- not an asteroid (will add it to exclusion list)
00:41:50.00 +50:22:44.0 -- not an asteroid (will add it to exclusion list)
00:35:37.92 +50:50:42.2 -- not an asteroid (will add it to exclusion list)
00:28:04.77 +48:42:28.0 -- not an asteroid (will add it to exclusion list)
00:27:47.01 +48:44:55.4 -- not an asteroid (will add it to exclusion list)
00:39:27.37 +49:30:14.0 -- not an asteroid (will add it to exclusion list)
00:40:07.46 +50:58:10.9 -- not an asteroid (will add it to exclusion list)
00:28:10.52 +50:28:13.3 -- not an asteroid (will add it to exclusion list)
00:40:25.51 +50:06:20.4 -- not an asteroid (will add it to exclusion list)
00:27:37.26 +46:39:48.3 -- not an asteroid (will add it to exclusion list)
00:37:13.26 +49:18:30.1 -- not an asteroid (will add it to exclusion list)
00:34:29.11 +49:44:40.1 -- not an asteroid (will add it to exclusion list)
00:40:02.38 +48:45:55.9 -- not an asteroid (will add it to exclusion list)
00:29:10.89 +50:35:55.5 -- not an asteroid (will add it to exclusion list)
00:40:22.63 +48:24:40.9 -- not an asteroid (will add it to exclusion list)
00:40:47.98 +50:22:54.8 -- not an asteroid (will add it to exclusion list)
00:39:44.84 +48:49:09.3 -- not an asteroid (will add it to exclusion list)
00:30:43.02 +50:40:39.6 -- not an asteroid (will add it to exclusion list)
00:41:56.98 +50:23:36.6 -- not an asteroid (will add it to exclusion list)
00:27:32.70 +47:03:25.6 -- not an asteroid (will add it to exclusion list)
00:31:52.49 +46:21:57.7 -- not an asteroid (will add it to exclusion list)
00:28:25.81 +46:51:48.6 -- not an asteroid (will add it to exclusion list)
00:33:42.49 +47:24:29.0 -- not an asteroid (will add it to exclusion list)
00:34:42.15 +50:28:57.4 -- not an asteroid (will add it to exclusion list)
00:27:48.06 +50:07:21.0 -- not an asteroid (will add it to exclusion list)
00:36:47.71 +50:42:53.9 -- not an asteroid (will add it to exclusion list)
00:31:47.45 +47:44:57.0 -- not an asteroid (will add it to exclusion list)
00:27:51.93 +46:50:39.7 -- not an asteroid (will add it to exclusion list)
00:33:00.95 +44:43:33.1 -- not an asteroid (will add it to exclusion list)
00:25:56.30 +50:25:36.6 -- not an asteroid (will add it to exclusion list)
00:32:36.67 +50:35:50.6 -- not an asteroid (will add it to exclusion list)
00:32:52.46 +47:20:32.6 -- not an asteroid (will add it to exclusion list)
00:36:54.48 +41:38:02.8 -- not an asteroid (will add it to exclusion list)
00:34:00.37 +47:26:14.4 -- not an asteroid (will add it to exclusion list)
00:33:23.87 +47:46:20.3 -- not an asteroid (will add it to exclusion list)
00:34:15.21 +45:44:27.2 -- not an asteroid (will add it to exclusion list)
00:27:06.72 +48:44:44.8 -- not an asteroid (will add it to exclusion list)
00:30:11.27 +47:42:51.6 -- not an asteroid (will add it to exclusion list)
00:33:30.94 +50:15:17.7 -- not an asteroid (will add it to exclusion list)
00:27:22.09 +50:06:14.5 -- not an asteroid (will add it to exclusion list)
00:34:06.84 +50:18:15.7 -- not an asteroid (will add it to exclusion list)
00:29:57.12 +50:51:20.4 -- not an asteroid (will add it to exclusion list)
00:26:39.99 +50:38:49.0 -- not an asteroid (will add it to exclusion list)
00:28:26.73 +47:32:06.4 -- not an asteroid (will add it to exclusion list)
00:32:50.24 +48:02:08.2 -- not an asteroid (will add it to exclusion list)
00:32:55.26 +50:52:16.6 -- not an asteroid (will add it to exclusion list)
00:33:11.55 +46:20:28.4 -- not an asteroid (will add it to exclusion list)
00:26:08.30 +50:36:53.2 -- not an asteroid (will add it to exclusion list)
00:31:26.81 +49:04:41.2 -- not an asteroid (will add it to exclusion list)
00:32:11.73 +50:25:33.3 -- not an asteroid (will add it to exclusion list)
00:40:02.87 +49:44:40.7 -- not an asteroid (will add it to exclusion list)
00:27:11.90 +50:08:47.8 -- not an asteroid (will add it to exclusion list)
00:31:49.76 +49:28:28.9 -- not an asteroid (will add it to exclusion list)
00:31:45.63 +45:04:58.0 -- not an asteroid (will add it to exclusion list)
00:42:16.59 +50:56:56.4 -- not an asteroid (will add it to exclusion list)
00:26:00.85 +49:45:49.8 -- not an asteroid (will add it to exclusion list)
00:36:15.62 +50:44:15.3 -- not an asteroid (will add it to exclusion list)
00:46:23.83 +50:54:06.0 -- not an asteroid (will add it to exclusion list)
00:40:56.78 +48:54:08.4 -- not an asteroid (will add it to exclusion list)
00:33:15.77 +49:37:33.7 -- not an asteroid (will add it to exclusion list)
00:32:21.55 +48:47:50.3 -- not an asteroid (will add it to exclusion list)
00:26:52.85 +50:27:01.0 -- not an asteroid (will add it to exclusion list)
00:34:21.95 +48:11:20.7 -- not an asteroid (will add it to exclusion list)
00:32:46.50 +50:19:34.2 -- not an asteroid (will add it to exclusion list)
00:32:11.08 +50:39:26.7 -- not an asteroid (will add it to exclusion list)
00:28:11.47 +50:09:06.6 -- not an asteroid (will add it to exclusion list)
00:27:46.97 +47:26:24.2 -- not an asteroid (will add it to exclusion list)
00:31:34.11 +50:08:03.2 -- not an asteroid (will add it to exclusion list)
00:30:19.59 +41:10:31.5 -- not an asteroid (will add it to exclusion list)
00:29:39.45 +50:03:41.8 -- not an asteroid (will add it to exclusion list)
00:31:05.24 +50:41:52.8 -- not an asteroid (will add it to exclusion list)
00:44:15.48 +50:16:51.3 -- not an asteroid (will add it to exclusion list)
00:44:01.83 +50:08:46.5 -- not an asteroid (will add it to exclusion list)
00:47:43.48 +49:58:08.9 -- not an asteroid (will add it to exclusion list)
00:29:39.05 +50:11:50.6 -- not an asteroid (will add it to exclusion list)
00:34:30.33 +50:35:31.2 -- not an asteroid (will add it to exclusion list)
00:38:29.50 +49:12:54.5 -- not an asteroid (will add it to exclusion list)
00:29:53.31 +48:07:15.7 -- not an asteroid (will add it to exclusion list)
00:28:47.26 +48:40:22.0 -- not an asteroid (will add it to exclusion list)
00:31:06.74 +48:27:58.3 -- not an asteroid (will add it to exclusion list)
00:31:34.55 +50:52:17.7 -- not an asteroid (will add it to exclusion list)
00:39:40.82 +49:10:20.1 -- not an asteroid (will add it to exclusion list)
00:31:10.55 +50:45:01.0 -- not an asteroid (will add it to exclusion list)
00:25:16.94 +50:35:20.6 -- not an asteroid (will add it to exclusion list)
00:28:10.60 +50:15:18.0 -- not an asteroid (will add it to exclusion list)
00:29:11.46 +47:45:53.1 -- not an asteroid (will add it to exclusion list)
00:33:16.34 +50:44:11.8 -- not an asteroid (will add it to exclusion list)
00:49:44.43 +41:02:37.4 -- not an asteroid (will add it to exclusion list)
00:30:07.34 +50:12:32.0 -- not an asteroid (will add it to exclusion list)
00:30:08.25 +49:12:19.3 -- not an asteroid (will add it to exclusion list)
00:29:53.44 +50:11:02.4 -- not an asteroid (will add it to exclusion list)
00:29:38.30 +42:09:08.4 -- not an asteroid (will add it to exclusion list)
00:34:40.69 +50:22:02.5 -- not an asteroid (will add it to exclusion list)
00:25:55.21 +49:48:43.2 -- not an asteroid (will add it to exclusion list)
00:28:45.96 +49:15:40.7 -- not an asteroid (will add it to exclusion list)
00:39:53.15 +50:41:16.4 -- not an asteroid (will add it to exclusion list)
00:43:01.54 +51:05:22.7 -- not an asteroid (will add it to exclusion list)
00:36:16.28 +49:53:12.7 -- not an asteroid (will add it to exclusion list)
00:32:35.02 +50:01:53.6 -- not an asteroid (will add it to exclusion list)
00:28:48.90 +43:56:36.2 -- not an asteroid (will add it to exclusion list)
00:27:29.41 +48:06:06.0 -- not an asteroid (will add it to exclusion list)
00:28:37.06 +46:18:09.9 -- not an asteroid (will add it to exclusion list)
00:46:52.35 +49:51:39.6 -- not an asteroid (will add it to exclusion list)
00:29:25.74 +49:41:21.6 -- not an asteroid (will add it to exclusion list)
00:27:06.50 +49:21:19.4 -- not an asteroid (will add it to exclusion list)
00:27:59.35 +50:27:49.0 -- not an asteroid (will add it to exclusion list)
00:42:50.51 +44:36:28.4 -- not an asteroid (will add it to exclusion list)
00:30:45.47 +45:18:50.6 -- not an asteroid (will add it to exclusion list)
00:36:25.68 +45:37:21.6 -- not an asteroid (will add it to exclusion list)
00:27:08.87 +49:17:55.6 -- not an asteroid (will add it to exclusion list)
00:26:33.82 +49:33:37.5 -- not an asteroid (will add it to exclusion list)
00:26:03.00 +50:33:43.8 -- not an asteroid (will add it to exclusion list)
00:51:20.35 +44:10:03.3 -- not an asteroid (will add it to exclusion list)
00:38:19.68 +50:40:00.1 -- not an asteroid (will add it to exclusion list)
00:32:45.06 +49:39:07.0 -- not an asteroid (will add it to exclusion list)
00:42:09.80 +50:45:46.9 -- not an asteroid (will add it to exclusion list)
00:30:23.89 +50:09:25.7 -- not an asteroid (will add it to exclusion list)
00:42:38.98 +46:09:02.8 -- not an asteroid (will add it to exclusion list)
00:33:43.39 +49:45:58.5 -- not an asteroid (will add it to exclusion list)
00:42:03.89 +50:21:14.9 -- not an asteroid (will add it to exclusion list)
00:32:30.81 +50:25:45.1 -- not an asteroid (will add it to exclusion list)
00:31:01.26 +47:46:46.6 -- not an asteroid (will add it to exclusion list)
00:29:14.34 +50:34:30.0 -- not an asteroid (will add it to exclusion list)
00:34:06.37 +43:14:12.9 -- not an asteroid (will add it to exclusion list)
00:29:48.22 +44:49:04.6 -- not an asteroid (will add it to exclusion list)
00:43:04.15 +51:04:00.3 -- not an asteroid (will add it to exclusion list)
00:30:17.47 +50:24:00.2 -- not an asteroid (will add it to exclusion list)
00:30:53.38 +47:32:54.7 -- not an asteroid (will add it to exclusion list)
00:26:55.34 +50:42:07.9 -- not an asteroid (will add it to exclusion list)
00:27:10.48 +49:24:48.3 -- not an asteroid (will add it to exclusion list)
00:26:22.18 +50:49:08.2 -- not an asteroid (will add it to exclusion list)
00:40:39.37 +50:04:30.0 -- not an asteroid (will add it to exclusion list)
00:38:24.31 +50:36:29.7 -- not an asteroid (will add it to exclusion list)
00:35:25.45 +50:14:35.3 -- not an asteroid (will add it to exclusion list)
00:28:47.38 +50:31:19.7 -- not an asteroid (will add it to exclusion list)
00:26:39.13 +50:15:24.8 -- not an asteroid (will add it to exclusion list)
00:32:49.84 +49:47:49.1 -- not an asteroid (will add it to exclusion list)
00:36:38.47 +42:10:48.9 -- not an asteroid (will add it to exclusion list)
00:39:19.76 +49:52:02.7 -- not an asteroid (will add it to exclusion list)
00:33:54.83 +50:30:03.4 -- not an asteroid (will add it to exclusion list)
00:30:47.73 +49:36:54.7 -- not an asteroid (will add it to exclusion list)
00:35:57.52 +44:26:05.3 -- not an asteroid (will add it to exclusion list)
00:38:45.82 +43:18:53.7 -- not an asteroid (will add it to exclusion list)
00:25:46.69 +49:53:38.0 -- not an asteroid (will add it to exclusion list)
00:31:56.93 +49:43:55.5 -- not an asteroid (will add it to exclusion list)
00:34:22.56 +49:51:07.5 -- not an asteroid (will add it to exclusion list)
00:26:47.68 +48:10:38.5 -- not an asteroid (will add it to exclusion list)
00:26:48.36 +48:10:42.3 -- not an asteroid (will add it to exclusion list)
00:32:17.11 +50:32:02.5 -- not an asteroid (will add it to exclusion list)
00:30:17.55 +44:55:50.5 -- not an asteroid (will add it to exclusion list)
00:27:52.04 +49:20:06.7 -- not an asteroid (will add it to exclusion list)
00:27:31.27 +47:36:58.9 -- not an asteroid (will add it to exclusion list)
00:33:57.83 +49:37:29.4 -- not an asteroid (will add it to exclusion list)
00:26:11.72 +50:49:43.5 -- not an asteroid (will add it to exclusion list)
00:32:27.85 +44:48:22.3 -- not an asteroid (will add it to exclusion list)
00:28:33.50 +44:52:49.4 -- not an asteroid (will add it to exclusion list)
00:33:24.86 +41:45:46.1 -- not an asteroid (will add it to exclusion list)
00:32:39.56 +50:18:05.6 -- not an asteroid (will add it to exclusion list)
00:29:11.93 +45:39:08.5 -- not an asteroid (will add it to exclusion list)
00:27:32.67 +49:57:23.8 -- not an asteroid (will add it to exclusion list)
00:27:43.85 +49:51:46.5 -- not an asteroid (will add it to exclusion list)
00:34:24.44 +50:39:44.8 -- not an asteroid (will add it to exclusion list)
00:27:06.77 +50:39:40.1 -- not an asteroid (will add it to exclusion list)
00:32:17.53 +50:32:04.4 -- not an asteroid (will add it to exclusion list)
00:29:26.36 +49:15:10.3 -- not an asteroid (will add it to exclusion list)
00:26:22.26 +49:05:47.5 -- not an asteroid (will add it to exclusion list)
01:55:41.06 +50:00:11.6 -- not an asteroid (will add it to exclusion list)
00:33:53.67 +50:00:13.5 -- not an asteroid (will add it to exclusion list)
00:42:59.68 +50:33:07.4 -- not an asteroid (will add it to exclusion list)
00:34:43.74 +43:16:57.3 -- not an asteroid (will add it to exclusion list)
00:30:06.90 +49:21:47.8 -- not an asteroid (will add it to exclusion list)
00:27:17.58 +48:55:28.3 -- not an asteroid (will add it to exclusion list)
00:29:40.13 +48:41:42.0 -- not an asteroid (will add it to exclusion list)
00:27:31.22 +46:55:30.7 -- not an asteroid (will add it to exclusion list)
00:32:44.96 +47:06:11.4 -- not an asteroid (will add it to exclusion list)
00:26:35.88 +48:52:42.5 -- not an asteroid (will add it to exclusion list)
00:28:50.50 +50:45:50.7 -- not an asteroid (will add it to exclusion list)
00:34:32.15 +43:30:48.6 -- not an asteroid (will add it to exclusion list)
00:27:55.45 +50:17:57.2 -- not an asteroid (will add it to exclusion list)
00:36:52.19 +49:27:44.5 -- not an asteroid (will add it to exclusion list)
00:27:26.86 +48:32:01.5 -- not an asteroid (will add it to exclusion list)
00:27:44.21 +50:49:28.8 -- not an asteroid (will add it to exclusion list)
00:32:55.99 +47:12:34.8 -- not an asteroid (will add it to exclusion list)
00:26:03.54 +49:35:56.5 -- not an asteroid (will add it to exclusion list)
00:40:15.10 +50:56:11.3 -- not an asteroid (will add it to exclusion list)
00:30:24.08 +41:20:21.0 -- not an asteroid (will add it to exclusion list)
00:28:14.64 +48:43:14.6 -- not an asteroid (will add it to exclusion list)
00:33:54.10 +47:12:58.0 -- not an asteroid (will add it to exclusion list)
00:25:35.00 +50:09:14.2 -- not an asteroid (will add it to exclusion list)
00:30:08.26 +49:34:49.0 -- not an asteroid (will add it to exclusion list)
00:38:56.24 +50:58:31.5 -- not an asteroid (will add it to exclusion list)
00:54:54.46 +41:10:28.6 -- not an asteroid (will add it to exclusion list)
01:20:28.68 +43:52:02.2 -- not an asteroid (will add it to exclusion list)
01:28:03.50 +49:29:53.6 -- not an asteroid (will add it to exclusion list)
01:16:04.64 +50:11:40.0 -- not an asteroid (will add it to exclusion list)
01:23:44.50 +49:24:07.3 -- not an asteroid (will add it to exclusion list)
01:17:55.72 +50:24:13.4 -- not an asteroid (will add it to exclusion list)
00:47:53.15 +48:30:44.7 -- not an asteroid (will add it to exclusion list)
01:10:12.11 +50:22:50.0 -- not an asteroid (will add it to exclusion list)
01:00:04.24 +48:40:23.8 -- not an asteroid (will add it to exclusion list)
01:31:54.80 +46:49:07.2 -- not an asteroid (will add it to exclusion list)
00:29:25.84 +48:36:05.5 -- not an asteroid (will add it to exclusion list)
00:49:14.16 +46:59:32.7 -- not an asteroid (will add it to exclusion list)
01:16:57.43 +49:34:43.7 -- not an asteroid (will add it to exclusion list)
01:17:29.78 +47:41:12.0 -- not an asteroid (will add it to exclusion list)
01:23:46.35 +47:16:25.4 -- not an asteroid (will add it to exclusion list)
00:56:40.47 +48:44:11.4 -- not an asteroid (will add it to exclusion list)
01:12:32.83 +50:51:24.3 -- not an asteroid (will add it to exclusion list)
01:20:54.65 +49:35:51.8 -- not an asteroid (will add it to exclusion list)
01:11:45.37 +43:16:18.1 -- not an asteroid (will add it to exclusion list)
00:49:08.09 +48:12:50.7 -- not an asteroid (will add it to exclusion list)
00:32:18.61 +50:27:38.4 -- not an asteroid (will add it to exclusion list)
00:38:53.25 +45:33:49.7 -- not an asteroid (will add it to exclusion list)
00:35:44.05 +50:33:08.7 -- not an asteroid (will add it to exclusion list)
00:57:28.45 +42:47:54.3 -- not an asteroid (will add it to exclusion list)
01:24:25.24 +45:36:20.1 -- not an asteroid (will add it to exclusion list)
01:06:04.74 +49:51:20.0 -- not an asteroid (will add it to exclusion list)
00:43:46.56 +51:02:35.7 -- not an asteroid (will add it to exclusion list)
01:14:22.24 +47:04:47.6 -- not an asteroid (will add it to exclusion list)
00:51:23.98 +49:09:52.9 -- not an asteroid (will add it to exclusion list)
01:37:29.69 +47:55:39.9 -- not an asteroid (will add it to exclusion list)
01:26:55.54 +47:24:02.8 -- not an asteroid (will add it to exclusion list)
01:36:40.37 +42:51:19.4 -- not an asteroid (will add it to exclusion list)
01:22:04.52 +46:06:40.4 -- not an asteroid (will add it to exclusion list)
01:31:04.14 +47:34:41.3 -- not an asteroid (will add it to exclusion list)
00:54:27.34 +43:55:38.0 -- not an asteroid (will add it to exclusion list)
01:00:48.10 +50:23:41.6 -- not an asteroid (will add it to exclusion list)
01:35:12.12 +46:33:47.6 -- not an asteroid (will add it to exclusion list)
01:06:23.29 +47:20:01.6 -- not an asteroid (will add it to exclusion list)
01:07:26.54 +45:36:35.6 -- not an asteroid (will add it to exclusion list)
01:21:37.14 +43:32:51.2 -- not an asteroid (will add it to exclusion list)
01:23:44.46 +45:52:03.1 -- not an asteroid (will add it to exclusion list)
01:00:21.25 +48:54:15.3 -- not an asteroid (will add it to exclusion list)
01:14:22.06 +49:58:28.9 -- not an asteroid (will add it to exclusion list)
00:57:04.39 +48:42:09.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:25:16.24 +50:31:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:16.94 +50:35:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:35.00 +50:09:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:46.69 +49:53:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:55.21 +49:48:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:56.30 +50:25:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:00.85 +49:45:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:03.00 +50:33:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:03.54 +49:35:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:08.30 +50:36:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:11.72 +50:49:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:22.18 +50:49:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:22.26 +49:05:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:33.82 +49:33:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:35.88 +48:52:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:39.13 +50:15:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:39.99 +50:38:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:47.68 +48:10:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:48.36 +48:10:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:49.68 +50:46:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:52.85 +50:27:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:55.34 +50:42:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:06.50 +49:21:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:06.72 +48:44:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:06.77 +50:39:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:08.87 +49:17:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:10.48 +49:24:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:11.90 +50:08:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:17.58 +48:55:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:22.09 +50:06:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:26.86 +48:32:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:29.41 +48:06:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:31.22 +46:55:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:31.27 +47:36:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:31.57 +48:49:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:32.67 +49:57:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:32.70 +47:03:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:37.26 +46:39:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:43.16 +48:12:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:43.85 +49:51:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:44.21 +50:49:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:46.97 +47:26:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:47.01 +48:44:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:48.06 +50:07:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:51.93 +46:50:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:52.04 +49:20:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:53.38 +46:08:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:54.37 +49:29:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:55.45 +50:17:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:59.35 +50:27:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:04.77 +48:42:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:05.04 +49:10:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:10.52 +50:28:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:10.60 +50:15:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:11.05 +50:28:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:11.47 +50:09:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:14.64 +48:43:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:25.81 +46:51:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:26.73 +47:32:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:33.50 +44:52:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:37.06 +46:18:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:39.06 +46:42:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:45.96 +49:15:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:47.26 +48:40:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:47.38 +50:31:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:48.90 +43:56:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:50.50 +50:45:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:53.47 +44:15:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:04.68 +46:31:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:05.57 +45:41:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:10.89 +50:35:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:11.46 +47:45:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:11.93 +45:39:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:14.34 +50:34:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:18.89 +46:12:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:25.74 +49:41:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:25.84 +48:36:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:26.36 +49:15:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:26.96 +42:33:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:32.62 +49:25:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:35.36 +48:43:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:38.30 +42:09:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:39.05 +50:11:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:39.45 +50:03:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:40.13 +48:41:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:41.18 +44:27:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:48.22 +44:49:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:49.36 +41:44:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:53.31 +48:07:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:53.44 +50:11:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:57.12 +50:51:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:58.05 +41:56:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:06.90 +49:21:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:07.34 +50:12:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:08.25 +49:12:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:08.26 +49:34:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:09.99 +42:25:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:11.27 +47:42:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:15.39 +42:20:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:17.47 +50:24:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:17.55 +44:55:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:19.59 +41:10:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:23.89 +50:09:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:24.08 +41:20:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:30.05 +44:28:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:43.02 +50:40:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:44.42 +47:48:53.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:45.47 +45:18:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:47.73 +49:36:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:50.10 +41:16:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:50.61 +43:43:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:51.74 +41:44:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:53.38 +47:32:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:55.16 +50:04:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:01.26 +47:46:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:05.24 +50:41:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:05.63 +46:50:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:06.74 +48:27:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:08.32 +42:49:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:10.55 +50:45:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:15.32 +44:21:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:22.40 +43:13:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:24.11 +44:25:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:26.81 +49:04:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:28.44 +49:04:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:34.11 +50:08:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:34.55 +50:52:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:35.16 +41:47:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:38.64 +43:08:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:41.15 +46:40:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:44.18 +50:02:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:45.08 +45:04:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:45.63 +45:04:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:47.45 +47:44:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:49.76 +49:28:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:52.49 +46:21:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:56.09 +42:33:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:56.93 +49:43:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:04.48 +43:46:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:07.96 +43:10:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:11.08 +50:39:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:11.73 +50:25:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:14.76 +43:02:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:17.11 +50:32:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:17.53 +50:32:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:18.61 +50:27:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:21.55 +48:47:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:27.85 +44:48:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:30.81 +50:25:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:34.15 +48:41:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:35.02 +50:01:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:36.67 +50:35:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:39.56 +50:18:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:39.63 +44:55:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:44.96 +47:06:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:45.06 +49:39:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:46.50 +50:19:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:49.44 +41:33:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:49.84 +49:47:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:50.08 +42:34:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:50.24 +48:02:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:50.53 +49:19:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:52.46 +47:20:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:54.29 +47:07:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:54.83 +41:50:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:55.07 +40:52:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:55.26 +50:52:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:55.99 +47:12:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:58.65 +43:15:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:00.95 +44:43:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:09.09 +42:48:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:09.14 +42:48:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:11.55 +46:20:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:15.77 +49:37:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:16.34 +50:44:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:22.70 +49:51:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:23.87 +47:46:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:24.86 +41:45:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:27.98 +44:19:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:28.11 +42:03:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:30.94 +50:15:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:35.66 +45:30:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:39.87 +44:07:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:42.49 +47:24:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:43.39 +49:45:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:43.43 +46:08:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:45.23 +42:24:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:45.26 +46:31:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:48.89 +43:21:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:53.67 +50:00:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:54.10 +47:12:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:54.83 +50:30:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:55.33 +48:39:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:55.78 +46:08:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:57.83 +49:37:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:58.45 +42:07:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:33:59.04 +50:30:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:00.37 +47:26:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:06.37 +43:14:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:06.84 +50:18:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:08.08 +44:36:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:14.62 +42:15:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:15.21 +45:44:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:21.95 +48:11:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:22.56 +49:51:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:24.44 +50:39:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:27.80 +49:19:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:28.88 +42:30:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:29.11 +49:44:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:30.33 +50:35:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:32.15 +43:30:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:34.69 +42:09:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:35.69 +47:34:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:40.69 +50:22:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:42.15 +50:28:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:42.75 +43:33:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:43.74 +43:16:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:52.33 +43:04:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:59.13 +43:38:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:00.04 +42:13:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:02.82 +42:35:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:07.66 +44:27:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:10.32 +45:16:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:25.34 +49:55:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:25.45 +50:14:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:36.91 +43:02:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:37.92 +50:50:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:38.15 +41:02:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:41.22 +45:20:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:43.70 +41:45:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:44.05 +50:33:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:44.15 +41:15:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:45.77 +49:23:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:45.81 +42:25:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:46.84 +41:39:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:55.68 +42:23:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:57.52 +44:26:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:00.05 +46:04:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:01.03 +41:23:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:05.33 +44:20:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:15.62 +50:44:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:16.28 +49:53:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:22.72 +44:29:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:22.78 +50:38:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:25.68 +45:37:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:25.74 +42:34:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:25.84 +41:03:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:27.59 +50:58:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:28.24 +44:27:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:29.53 +49:32:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:34.59 +49:09:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:36.31 +41:42:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:36.73 +46:12:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:38.47 +42:10:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:47.71 +50:42:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:48.66 +50:42:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:49.40 +44:35:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:52.19 +49:27:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:54.15 +48:50:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:54.48 +41:38:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:36:55.07 +42:20:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:13.26 +49:18:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:13.63 +44:16:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:19.26 +45:51:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:27.73 +42:03:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:30.07 +45:50:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:32.75 +42:53:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:33.86 +41:55:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:34.52 +44:27:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:40.43 +46:38:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:41.55 +47:58:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:48.84 +43:51:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:58.47 +42:40:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:14.08 +42:16:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:17.33 +43:36:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:19.68 +50:40:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:24.31 +50:36:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:24.78 +44:16:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:29.50 +49:12:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:31.88 +41:33:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:32.84 +43:35:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:38.51 +43:48:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:39.17 +43:48:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:45.74 +43:49:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:45.82 +43:18:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:46.51 +46:52:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:48.42 +46:30:21.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:51.55 +43:44:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:53.25 +45:33:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:56.24 +50:58:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:38:58.18 +43:00:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:02.12 +49:30:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:05.16 +40:55:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:07.27 +48:10:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:18.12 +49:31:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:18.67 +48:30:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:19.76 +49:52:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:19.95 +41:55:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:21.80 +43:26:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:25.42 +47:25:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:27.37 +49:30:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:40.36 +42:36:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:40.82 +49:10:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:41.74 +41:26:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:44.84 +48:49:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:53.15 +50:41:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:02.38 +48:45:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:02.87 +49:44:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:03.46 +41:19:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:04.02 +42:13:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:06.38 +42:22:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:07.46 +50:58:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:12.14 +46:51:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:14.45 +44:46:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:15.10 +50:56:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:15.19 +50:49:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:19.55 +43:04:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:22.63 +48:24:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:24.37 +44:01:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:25.51 +50:06:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:33.46 +44:20:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:38.56 +43:06:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:39.37 +50:04:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:42.06 +48:34:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:42.40 +48:48:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:45.58 +42:16:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:46.85 +50:18:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:47.98 +50:22:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:54.80 +43:18:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:55.67 +40:57:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:56.78 +48:54:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:58.52 +41:43:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:18.74 +44:10:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:21.83 +46:23:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:27.25 +42:12:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:27.98 +44:06:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:37.03 +41:40:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:47.58 +42:40:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:50.00 +50:22:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:56.98 +50:23:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:01.53 +42:36:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:03.89 +50:21:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:09.80 +50:45:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:10.50 +41:26:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:11.80 +48:53:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:16.59 +50:56:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:19.61 +42:25:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:21.35 +45:04:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:24.39 +43:09:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:30.39 +44:32:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:32.09 +40:57:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:36.20 +44:15:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:38.80 +49:34:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:38.98 +46:09:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:44.69 +49:22:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:50.51 +44:36:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:52.87 +43:18:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:58.20 +40:58:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:59.68 +50:33:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:42:59.97 +41:05:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:00.26 +41:28:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:01.54 +51:05:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:04.15 +51:04:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:11.12 +41:36:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:25.55 +41:24:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:44.55 +41:04:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:46.56 +51:02:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:43:47.17 +44:05:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:01.83 +50:08:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:05.02 +42:19:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:08.79 +42:27:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:15.48 +50:16:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:50.41 +41:06:08.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:52.14 +46:14:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:52.33 +41:25:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:44:53.46 +49:53:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:08.14 +46:22:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:09.49 +48:17:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:14.07 +41:03:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:30.88 +40:58:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:32.07 +42:27:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:35.47 +43:34:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:46.38 +42:25:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:56.25 +50:23:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:17.98 +50:52:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:22.18 +50:04:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:23.83 +50:54:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:26.17 +45:54:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:32.24 +41:51:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:37.44 +41:08:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:38.86 +42:57:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:51.43 +42:18:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:52.35 +49:51:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:54.07 +49:11:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:20.19 +43:53:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:43.48 +49:58:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:49.56 +48:00:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:50.79 +50:26:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:53.15 +48:30:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:55.32 +49:51:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:43.63 +50:52:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:08.09 +48:12:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:14.16 +46:59:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:17.74 +42:47:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:36.89 +41:29:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:44.43 +41:02:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:53.72 +41:14:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:57.43 +45:10:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:14.82 +41:02:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:20.35 +44:10:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:23.98 +49:09:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:35.56 +41:37:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:55.88 +51:02:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:35.41 +44:54:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:57.44 +50:46:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:27.34 +43:55:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:37.50 +49:28:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:44.06 +41:23:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:54:54.46 +41:10:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:13.37 +46:39:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:15.09 +49:39:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:55:48.81 +44:10:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:40.47 +48:44:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:54.71 +41:31:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:04.39 +48:42:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:28.45 +42:47:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:58:20.83 +49:25:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:04.24 +48:40:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:20.71 +41:01:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:21.25 +48:54:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:00:48.10 +50:23:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:02:24.96 +47:26:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:03:40.80 +48:10:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:05:51.98 +48:50:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:04.74 +49:51:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:06:23.29 +47:20:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:07.67 +43:02:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:07:26.54 +45:36:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:09:27.78 +42:40:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:12.11 +50:22:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:12.93 +49:10:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:10:43.33 +43:20:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:14.09 +50:23:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:11:45.37 +43:16:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:12:32.83 +50:51:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:13:46.30 +46:34:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:04.52 +47:52:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:22.06 +49:58:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:14:22.24 +47:04:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:15:42.26 +46:12:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:04.64 +50:11:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:19.81 +47:27:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:16:57.43 +49:34:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:29.78 +47:41:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:17:55.72 +50:24:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:19:23.91 +48:26:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:28.68 +43:52:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:20:54.65 +49:35:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:11.80 +48:29:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:21:37.14 +43:32:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:22:04.52 +46:06:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:44.46 +45:52:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:44.50 +49:24:07.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:23:46.35 +47:16:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:24:25.24 +45:36:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:25:48.53 +46:24:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:27.60 +49:53:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
01:26:55.54 +47:24:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:03.50 +49:29:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:28:47.66 +44:16:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:29:26.69 +46:27:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:04.14 +47:34:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:54.80 +46:49:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
01:31:58.34 +45:46:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:33:35.62 +46:31:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
01:35:12.12 +46:33:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
01:36:40.37 +42:51:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
01:37:29.69 +47:55:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
01:51:23.52 +49:56:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
01:55:41.06 +50:00:11.6 -- 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)
00:25:16.24 +50:31:57.6 -- not a known variable star
00:25:16.94 +50:35:20.6 -- not a known variable star
00:25:35.00 +50:09:14.2 -- not a known variable star
00:25:46.69 +49:53:38.0 -- not a known variable star
00:25:55.21 +49:48:43.2 -- a known variable star
00:25:56.30 +50:25:36.6 -- a known variable star
00:26:00.85 +49:45:49.8 -- not a known variable star
00:26:03.00 +50:33:43.8 -- not a known variable star
00:26:03.54 +49:35:56.5 -- not a known variable star
00:26:08.30 +50:36:53.2 -- not a known variable star
00:26:11.72 +50:49:43.5 -- not a known variable star
00:26:22.18 +50:49:08.2 -- not a known variable star
00:26:22.26 +49:05:47.5 -- not a known variable star
00:26:33.82 +49:33:37.5 -- not a known variable star
00:26:35.88 +48:52:42.5 -- not a known variable star
00:26:39.13 +50:15:24.8 -- not a known variable star
00:26:39.99 +50:38:49.0 -- not a known variable star
00:26:47.68 +48:10:38.5 -- not a known variable star
00:26:48.36 +48:10:42.3 -- not a known variable star
00:26:49.68 +50:46:16.7 -- not a known variable star
00:26:52.85 +50:27:01.0 -- not a known variable star
00:26:55.34 +50:42:07.9 -- not a known variable star
00:27:06.50 +49:21:19.4 -- not a known variable star
00:27:06.72 +48:44:44.8 -- not a known variable star
00:27:06.77 +50:39:40.1 -- not a known variable star
00:27:08.87 +49:17:55.6 -- not a known variable star
00:27:10.48 +49:24:48.3 -- not a known variable star
00:27:11.90 +50:08:47.8 -- not a known variable star
00:27:17.58 +48:55:28.3 -- a known variable star
00:27:22.09 +50:06:14.5 -- not a known variable star
00:27:26.86 +48:32:01.5 -- not a known variable star
00:27:29.41 +48:06:06.0 -- not a known variable star
00:27:31.22 +46:55:30.7 -- not a known variable star
00:27:31.27 +47:36:58.9 -- not a known variable star
00:27:31.57 +48:49:15.5 -- not a known variable star
00:27:32.67 +49:57:23.8 -- not a known variable star
00:27:32.70 +47:03:25.6 -- not a known variable star
00:27:37.26 +46:39:48.3 -- not a known variable star
00:27:43.16 +48:12:16.1 -- not a known variable star
00:27:43.85 +49:51:46.5 -- not a known variable star
00:27:44.21 +50:49:28.8 -- not a known variable star
00:27:46.97 +47:26:24.2 -- not a known variable star
00:27:47.01 +48:44:55.4 -- not a known variable star
00:27:48.06 +50:07:21.0 -- not a known variable star
00:27:51.93 +46:50:39.7 -- not a known variable star
00:27:52.04 +49:20:06.7 -- not a known variable star
00:27:53.38 +46:08:08.5 -- not a known variable star
00:27:54.37 +49:29:44.4 -- not a known variable star
00:27:55.45 +50:17:57.2 -- not a known variable star
00:27:59.35 +50:27:49.0 -- not a known variable star
00:28:04.77 +48:42:28.0 -- not a known variable star
00:28:05.04 +49:10:14.5 -- not a known variable star
00:28:10.52 +50:28:13.3 -- not a known variable star
00:28:10.60 +50:15:18.0 -- not a known variable star
00:28:11.05 +50:28:08.9 -- not a known variable star
00:28:11.47 +50:09:06.6 -- not a known variable star
00:28:14.64 +48:43:14.6 -- not a known variable star
00:28:25.81 +46:51:48.6 -- not a known variable star
00:28:26.73 +47:32:06.4 -- not a known variable star
00:28:33.50 +44:52:49.4 -- not a known variable star
00:28:37.06 +46:18:09.9 -- not a known variable star
00:28:39.06 +46:42:07.2 -- a known variable star
00:28:45.96 +49:15:40.7 -- not a known variable star
00:28:47.26 +48:40:22.0 -- not a known variable star
00:28:47.38 +50:31:19.7 -- not a known variable star
00:28:48.90 +43:56:36.2 -- not a known variable star
00:28:50.50 +50:45:50.7 -- not a known variable star
00:28:53.47 +44:15:58.5 -- not a known variable star
00:29:04.68 +46:31:28.9 -- not a known variable star
00:29:05.57 +45:41:25.8 -- not a known variable star
00:29:10.89 +50:35:55.5 -- not a known variable star
00:29:11.46 +47:45:53.1 -- not a known variable star
00:29:11.93 +45:39:08.5 -- not a known variable star
00:29:14.34 +50:34:30.0 -- not a known variable star
00:29:18.89 +46:12:00.8 -- not a known variable star
00:29:25.74 +49:41:21.6 -- not a known variable star
00:29:25.84 +48:36:05.5 -- not a known variable star
00:29:26.36 +49:15:10.3 -- not a known variable star
00:29:26.96 +42:33:03.3 -- not a known variable star
00:29:32.62 +49:25:24.8 -- a known variable star
00:29:35.36 +48:43:49.5 -- not a known variable star
00:29:38.30 +42:09:08.4 -- not a known variable star
00:29:39.05 +50:11:50.6 -- not a known variable star
00:29:39.45 +50:03:41.8 -- not a known variable star
00:29:40.13 +48:41:42.0 -- not a known variable star
00:29:41.18 +44:27:34.1 -- not a known variable star
00:29:48.22 +44:49:04.6 -- not a known variable star
00:29:49.36 +41:44:42.3 -- not a known variable star
00:29:53.31 +48:07:15.7 -- a known variable star
00:29:53.44 +50:11:02.4 -- not a known variable star
00:29:57.12 +50:51:20.4 -- not a known variable star
00:29:58.05 +41:56:50.4 -- not a known variable star
00:30:06.90 +49:21:47.8 -- not a known variable star
00:30:07.34 +50:12:32.0 -- not a known variable star
00:30:08.25 +49:12:19.3 -- not a known variable star
00:30:08.26 +49:34:49.0 -- not a known variable star
00:30:09.99 +42:25:39.4 -- not a known variable star
00:30:11.27 +47:42:51.6 -- not a known variable star
00:30:15.39 +42:20:16.9 -- not a known variable star
00:30:17.47 +50:24:00.2 -- not a known variable star
00:30:17.55 +44:55:50.5 -- not a known variable star
00:30:19.59 +41:10:31.5 -- a known variable star
00:30:23.89 +50:09:25.7 -- not a known variable star
00:30:24.08 +41:20:21.0 -- not a known variable star
00:30:30.05 +44:28:06.2 -- not a known variable star
00:30:43.02 +50:40:39.6 -- a known variable star
00:30:44.42 +47:48:53.3 -- not a known variable star
00:30:45.47 +45:18:50.6 -- not a known variable star
00:30:47.73 +49:36:54.7 -- not a known variable star
00:30:50.10 +41:16:32.5 -- not a known variable star
00:30:50.61 +43:43:00.9 -- not a known variable star
00:30:51.74 +41:44:46.9 -- not a known variable star
00:30:53.38 +47:32:54.7 -- not a known variable star
00:30:55.16 +50:04:24.3 -- not a known variable star
00:31:01.26 +47:46:46.6 -- a known variable star
00:31:05.24 +50:41:52.8 -- a known variable star
00:31:05.63 +46:50:59.2 -- not a known variable star
00:31:06.74 +48:27:58.3 -- a known variable star
00:31:08.32 +42:49:07.5 -- not a known variable star
00:31:10.55 +50:45:01.0 -- not a known variable star
00:31:15.32 +44:21:00.0 -- not a known variable star
00:31:22.40 +43:13:28.5 -- not a known variable star
00:31:24.11 +44:25:24.4 -- not a known variable star
00:31:26.81 +49:04:41.2 -- not a known variable star
00:31:28.44 +49:04:22.2 -- a known variable star
00:31:34.11 +50:08:03.2 -- not a known variable star
00:31:34.55 +50:52:17.7 -- not a known variable star
00:31:35.16 +41:47:32.7 -- not a known variable star
00:31:38.64 +43:08:45.1 -- not a known variable star
00:31:41.15 +46:40:05.1 -- a known variable star
00:31:44.18 +50:02:56.2 -- not a known variable star
00:31:45.08 +45:04:33.0 -- not a known variable star
00:31:45.63 +45:04:58.0 -- not a known variable star
00:31:47.45 +47:44:57.0 -- a known variable star
00:31:49.76 +49:28:28.9 -- not a known variable star
00:31:52.49 +46:21:57.7 -- not a known variable star
00:31:56.09 +42:33:26.3 -- not a known variable star
00:31:56.93 +49:43:55.5 -- not a known variable star
00:32:04.48 +43:46:41.9 -- not a known variable star
00:32:07.96 +43:10:49.6 -- not a known variable star
00:32:11.08 +50:39:26.7 -- not a known variable star
00:32:11.73 +50:25:33.3 -- not a known variable star
00:32:14.76 +43:02:06.8 -- not a known variable star
00:32:17.11 +50:32:02.5 -- not a known variable star
00:32:17.53 +50:32:04.4 -- not a known variable star
00:32:18.61 +50:27:38.4 -- not a known variable star
00:32:21.55 +48:47:50.3 -- not a known variable star
00:32:27.85 +44:48:22.3 -- not a known variable star
00:32:30.81 +50:25:45.1 -- a known variable star
00:32:34.15 +48:41:56.2 -- not a known variable star
00:32:35.02 +50:01:53.6 -- not a known variable star
00:32:36.67 +50:35:50.6 -- not a known variable star
00:32:39.56 +50:18:05.6 -- not a known variable star
00:32:39.63 +44:55:13.9 -- not a known variable star
00:32:44.96 +47:06:11.4 -- not a known variable star
00:32:45.06 +49:39:07.0 -- not a known variable star
00:32:46.50 +50:19:34.2 -- not a known variable star
00:32:49.44 +41:33:51.5 -- not a known variable star
00:32:49.84 +49:47:49.1 -- not a known variable star
00:32:50.08 +42:34:54.4 -- not a known variable star
00:32:50.24 +48:02:08.2 -- not a known variable star
00:32:50.53 +49:19:44.5 -- a known variable star
00:32:52.46 +47:20:32.6 -- not a known variable star
00:32:54.29 +47:07:43.0 -- not a known variable star
00:32:54.83 +41:50:09.4 -- not a known variable star
00:32:55.07 +40:52:22.6 -- not a known variable star
00:32:55.26 +50:52:16.6 -- not a known variable star
00:32:55.99 +47:12:34.8 -- a known variable star
00:32:58.65 +43:15:23.0 -- a known variable star
00:33:00.95 +44:43:33.1 -- not a known variable star
00:33:09.09 +42:48:22.6 -- not a known variable star
00:33:09.14 +42:48:18.3 -- not a known variable star
00:33:11.55 +46:20:28.4 -- not a known variable star
00:33:15.77 +49:37:33.7 -- not a known variable star
00:33:16.34 +50:44:11.8 -- not a known variable star
00:33:22.70 +49:51:24.6 -- a known variable star
00:33:23.87 +47:46:20.3 -- not a known variable star
00:33:24.86 +41:45:46.1 -- not a known variable star
00:33:27.98 +44:19:03.1 -- not a known variable star
00:33:28.11 +42:03:50.7 -- not a known variable star
00:33:30.94 +50:15:17.7 -- not a known variable star
00:33:35.66 +45:30:31.1 -- not a known variable star
00:33:39.87 +44:07:45.0 -- not a known variable star
00:33:42.49 +47:24:29.0 -- not a known variable star
00:33:43.39 +49:45:58.5 -- not a known variable star
00:33:43.43 +46:08:52.8 -- not a known variable star
00:33:45.23 +42:24:49.0 -- not a known variable star
00:33:45.26 +46:31:47.2 -- not a known variable star
00:33:48.89 +43:21:36.8 -- not a known variable star
00:33:53.67 +50:00:13.5 -- not a known variable star
00:33:54.10 +47:12:58.0 -- not a known variable star
00:33:54.83 +50:30:03.4 -- not a known variable star
00:33:55.33 +48:39:10.4 -- not a known variable star
00:33:55.78 +46:08:48.1 -- a known variable star
00:33:57.83 +49:37:29.4 -- not a known variable star
00:33:58.45 +42:07:29.3 -- not a known variable star
00:33:59.04 +50:30:22.6 -- not a known variable star
00:34:00.37 +47:26:14.4 -- not a known variable star
00:34:06.37 +43:14:12.9 -- not a known variable star
00:34:06.84 +50:18:15.7 -- not a known variable star
00:34:08.08 +44:36:16.1 -- not a known variable star
00:34:14.62 +42:15:49.1 -- a known variable star
00:34:15.21 +45:44:27.2 -- not a known variable star
00:34:21.95 +48:11:20.7 -- not a known variable star
00:34:22.56 +49:51:07.5 -- not a known variable star
00:34:24.44 +50:39:44.8 -- not a known variable star
00:34:27.80 +49:19:12.3 -- not a known variable star
00:34:28.88 +42:30:06.4 -- not a known variable star
00:34:29.11 +49:44:40.1 -- not a known variable star
00:34:30.33 +50:35:31.2 -- not a known variable star
00:34:32.15 +43:30:48.6 -- not a known variable star
00:34:34.69 +42:09:25.3 -- not a known variable star
00:34:35.69 +47:34:42.4 -- not a known variable star
00:34:40.69 +50:22:02.5 -- a known variable star
00:34:42.15 +50:28:57.4 -- not a known variable star
00:34:42.75 +43:33:40.6 -- not a known variable star
00:34:43.74 +43:16:57.3 -- not a known variable star
00:34:52.33 +43:04:54.3 -- not a known variable star
00:34:59.13 +43:38:26.1 -- not a known variable star
00:35:00.04 +42:13:42.7 -- not a known variable star
00:35:02.82 +42:35:09.7 -- not a known variable star
00:35:07.66 +44:27:31.7 -- not a known variable star
00:35:10.32 +45:16:12.0 -- not a known variable star
00:35:25.34 +49:55:43.8 -- not a known variable star
00:35:25.45 +50:14:35.3 -- not a known variable star
00:35:36.91 +43:02:35.6 -- not a known variable star
00:35:37.92 +50:50:42.2 -- not a known variable star
00:35:38.15 +41:02:02.2 -- not a known variable star
00:35:41.22 +45:20:46.4 -- not a known variable star
00:35:43.70 +41:45:08.4 -- not a known variable star
00:35:44.05 +50:33:08.7 -- not a known variable star
00:35:44.15 +41:15:09.3 -- not a known variable star
00:35:45.77 +49:23:12.7 -- not a known variable star
00:35:45.81 +42:25:30.9 -- not a known variable star
00:35:46.84 +41:39:44.1 -- not a known variable star
00:35:55.68 +42:23:43.1 -- not a known variable star
00:35:57.52 +44:26:05.3 -- not a known variable star
00:36:00.05 +46:04:24.3 -- a known variable star
00:36:01.03 +41:23:26.6 -- not a known variable star
00:36:05.33 +44:20:32.8 -- not a known variable star
00:36:15.62 +50:44:15.3 -- not a known variable star
00:36:16.28 +49:53:12.7 -- not a known variable star
00:36:22.72 +44:29:44.7 -- not a known variable star
00:36:22.78 +50:38:17.7 -- not a known variable star
00:36:25.68 +45:37:21.6 -- not a known variable star
00:36:25.74 +42:34:30.4 -- not a known variable star
00:36:25.84 +41:03:26.3 -- not a known variable star
00:36:27.59 +50:58:06.8 -- not a known variable star
00:36:28.24 +44:27:45.7 -- not a known variable star
00:36:29.53 +49:32:09.7 -- not a known variable star
00:36:34.59 +49:09:03.9 -- a known variable star
00:36:36.31 +41:42:11.7 -- a known variable star
00:36:36.73 +46:12:55.9 -- not a known variable star
00:36:38.47 +42:10:48.9 -- not a known variable star
00:36:47.71 +50:42:53.9 -- not a known variable star
00:36:48.66 +50:42:52.3 -- not a known variable star
00:36:49.40 +44:35:15.5 -- not a known variable star
00:36:52.19 +49:27:44.5 -- not a known variable star
00:36:54.15 +48:50:38.7 -- not a known variable star
00:36:54.48 +41:38:02.8 -- not a known variable star
00:36:55.07 +42:20:24.3 -- a known variable star
00:37:13.26 +49:18:30.1 -- not a known variable star
00:37:13.63 +44:16:56.6 -- not a known variable star
00:37:19.26 +45:51:17.0 -- not a known variable star
00:37:27.73 +42:03:43.4 -- not a known variable star
00:37:30.07 +45:50:30.3 -- not a known variable star
00:37:32.75 +42:53:15.8 -- not a known variable star
00:37:33.86 +41:55:06.5 -- not a known variable star
00:37:34.52 +44:27:48.1 -- not a known variable star
00:37:40.43 +46:38:53.5 -- not a known variable star
00:37:41.55 +47:58:23.2 -- not a known variable star
00:37:48.84 +43:51:08.4 -- not a known variable star
00:37:58.47 +42:40:08.9 -- not a known variable star
00:38:14.08 +42:16:52.0 -- not a known variable star
00:38:17.33 +43:36:12.0 -- not a known variable star
00:38:19.68 +50:40:00.1 -- not a known variable star
00:38:24.31 +50:36:29.7 -- a known variable star
00:38:24.78 +44:16:41.4 -- not a known variable star
00:38:29.50 +49:12:54.5 -- a known variable star
00:38:31.88 +41:33:57.7 -- not a known variable star
00:38:32.84 +43:35:18.0 -- a known variable star
00:38:38.51 +43:48:31.3 -- not a known variable star
00:38:39.17 +43:48:36.1 -- not a known variable star
00:38:45.74 +43:49:49.7 -- not a known variable star
00:38:45.82 +43:18:53.7 -- not a known variable star
00:38:46.51 +46:52:37.6 -- not a known variable star
00:38:48.42 +46:30:21.2 -- not a known variable star
00:38:51.55 +43:44:31.9 -- not a known variable star
00:38:53.25 +45:33:49.7 -- a known variable star
00:38:56.24 +50:58:31.5 -- not a known variable star
00:38:58.18 +43:00:35.8 -- not a known variable star
00:39:02.12 +49:30:32.7 -- not a known variable star
00:39:05.16 +40:55:41.8 -- not a known variable star
00:39:07.27 +48:10:19.6 -- not a known variable star
00:39:18.12 +49:31:27.4 -- not a known variable star
00:39:18.67 +48:30:25.9 -- not a known variable star
00:39:19.76 +49:52:02.7 -- not a known variable star
00:39:19.95 +41:55:34.6 -- not a known variable star
00:39:21.80 +43:26:05.0 -- not a known variable star
00:39:25.42 +47:25:28.8 -- a known variable star
00:39:27.37 +49:30:14.0 -- not a known variable star
00:39:40.36 +42:36:07.8 -- not a known variable star
00:39:40.82 +49:10:20.1 -- not a known variable star
00:39:41.74 +41:26:54.8 -- not a known variable star
00:39:44.84 +48:49:09.3 -- not a known variable star
00:39:53.15 +50:41:16.4 -- not a known variable star
00:40:02.38 +48:45:55.9 -- not a known variable star
00:40:02.87 +49:44:40.7 -- not a known variable star
00:40:03.46 +41:19:01.0 -- not a known variable star
00:40:04.02 +42:13:37.6 -- not a known variable star
00:40:06.38 +42:22:42.1 -- not a known variable star
00:40:07.46 +50:58:10.9 -- not a known variable star
00:40:12.14 +46:51:11.0 -- not a known variable star
00:40:14.45 +44:46:47.0 -- not a known variable star
00:40:15.10 +50:56:11.3 -- not a known variable star
00:40:15.19 +50:49:23.2 -- not a known variable star
00:40:19.55 +43:04:59.3 -- not a known variable star
00:40:22.63 +48:24:40.9 -- not a known variable star
00:40:24.37 +44:01:18.8 -- not a known variable star
00:40:25.51 +50:06:20.4 -- a known variable star
00:40:33.46 +44:20:49.8 -- not a known variable star
00:40:38.56 +43:06:25.1 -- not a known variable star
00:40:39.37 +50:04:30.0 -- not a known variable star
00:40:42.06 +48:34:27.0 -- not a known variable star
00:40:42.40 +48:48:37.5 -- not a known variable star
00:40:45.58 +42:16:48.8 -- not a known variable star
00:40:46.85 +50:18:46.7 -- not a known variable star
00:40:47.98 +50:22:54.8 -- not a known variable star
00:40:54.80 +43:18:07.5 -- not a known variable star
00:40:55.67 +40:57:43.4 -- a known variable star
00:40:56.78 +48:54:08.4 -- not a known variable star
00:40:58.52 +41:43:55.5 -- not a known variable star
00:41:18.74 +44:10:21.0 -- not a known variable star
00:41:21.83 +46:23:45.3 -- not a known variable star
00:41:27.25 +42:12:52.2 -- not a known variable star
00:41:27.98 +44:06:28.9 -- not a known variable star
00:41:37.03 +41:40:20.0 -- not a known variable star
00:41:47.58 +42:40:34.2 -- not a known variable star
00:41:50.00 +50:22:44.0 -- not a known variable star
00:41:56.98 +50:23:36.6 -- not a known variable star
00:42:01.53 +42:36:59.2 -- not a known variable star
00:42:03.89 +50:21:14.9 -- not a known variable star
00:42:09.80 +50:45:46.9 -- not a known variable star
00:42:10.50 +41:26:20.5 -- not a known variable star
00:42:11.80 +48:53:19.9 -- a known variable star
00:42:16.59 +50:56:56.4 -- not a known variable star
00:42:19.61 +42:25:25.9 -- not a known variable star
00:42:21.35 +45:04:14.7 -- not a known variable star
00:42:24.39 +43:09:57.8 -- not a known variable star
00:42:30.39 +44:32:12.6 -- not a known variable star
00:42:32.09 +40:57:18.8 -- not a known variable star
00:42:36.20 +44:15:33.5 -- not a known variable star
00:42:38.80 +49:34:51.5 -- not a known variable star
00:42:38.98 +46:09:02.8 -- not a known variable star
00:42:44.69 +49:22:32.1 -- not a known variable star
00:42:50.51 +44:36:28.4 -- not a known variable star
00:42:52.87 +43:18:59.8 -- not a known variable star
00:42:58.20 +40:58:58.5 -- a known object
00:42:59.68 +50:33:07.4 -- not a known variable star
00:42:59.97 +41:05:53.6 -- not a known variable star
00:43:00.26 +41:28:54.6 -- not a known variable star
00:43:01.54 +51:05:22.7 -- a known variable star
00:43:04.15 +51:04:00.3 -- not a known variable star
00:43:11.12 +41:36:14.9 -- not a known variable star
00:43:25.55 +41:24:23.1 -- not a known variable star
00:43:44.55 +41:04:55.1 -- not a known variable star
00:43:46.56 +51:02:35.7 -- not a known variable star
00:43:47.17 +44:05:58.5 -- not a known variable star
00:44:01.83 +50:08:46.5 -- not a known variable star
00:44:05.02 +42:19:57.0 -- not a known variable star
00:44:08.79 +42:27:38.3 -- not a known variable star
00:44:15.48 +50:16:51.3 -- not a known variable star
00:44:50.41 +41:06:08.0 -- not a known variable star
00:44:52.14 +46:14:18.9 -- not a known variable star
00:44:52.33 +41:25:03.3 -- not a known variable star
00:44:53.46 +49:53:06.5 -- not a known variable star
00:45:08.14 +46:22:02.1 -- not a known variable star
00:45:09.49 +48:17:57.1 -- not a known variable star
00:45:14.07 +41:03:01.6 -- not a known variable star
00:45:30.88 +40:58:40.2 -- not a known variable star
00:45:32.07 +42:27:42.3 -- not a known variable star
00:45:35.47 +43:34:46.5 -- not a known variable star
00:45:46.38 +42:25:21.5 -- not a known variable star
00:45:56.25 +50:23:15.7 -- a known variable star
00:46:17.98 +50:52:33.5 -- not a known variable star
00:46:22.18 +50:04:38.5 -- not a known variable star
00:46:23.83 +50:54:06.0 -- not a known variable star
00:46:26.17 +45:54:34.7 -- not a known variable star
00:46:32.24 +41:51:49.3 -- not a known variable star
00:46:37.44 +41:08:56.1 -- not a known variable star
00:46:38.86 +42:57:47.0 -- not a known variable star
00:46:51.43 +42:18:06.4 -- not a known variable star
00:46:52.35 +49:51:39.6 -- not a known variable star
00:46:54.07 +49:11:17.1 -- not a known variable star
00:47:20.19 +43:53:19.0 -- not a known variable star
00:47:43.48 +49:58:08.9 -- not a known variable star
00:47:49.56 +48:00:39.9 -- not a known variable star
00:47:50.79 +50:26:10.8 -- not a known variable star
00:47:53.15 +48:30:44.7 -- a known variable star
00:47:55.32 +49:51:36.5 -- a known variable star
00:48:43.63 +50:52:13.4 -- not a known variable star
00:49:08.09 +48:12:50.7 -- a known variable star
00:49:14.16 +46:59:32.7 -- a known variable star
00:49:17.74 +42:47:31.3 -- not a known variable star
00:49:36.89 +41:29:06.4 -- not a known variable star
00:49:44.43 +41:02:37.4 -- a known variable star
00:49:53.72 +41:14:09.2 -- not a known variable star
00:49:57.43 +45:10:25.3 -- not a known variable star
00:51:14.82 +41:02:16.8 -- not a known variable star
00:51:20.35 +44:10:03.3 -- not a known variable star
00:51:23.98 +49:09:52.9 -- a known variable star
00:51:35.56 +41:37:04.6 -- not a known variable star
00:51:55.88 +51:02:22.0 -- not a known variable star
00:52:35.41 +44:54:12.9 -- not a known variable star
00:52:57.44 +50:46:08.6 -- not a known variable star
00:54:27.34 +43:55:38.0 -- a known variable star
00:54:37.50 +49:28:21.1 -- not a known variable star
00:54:44.06 +41:23:44.1 -- not a known variable star
00:54:54.46 +41:10:28.6 -- not a known variable star
00:55:13.37 +46:39:01.7 -- not a known variable star
00:55:15.09 +49:39:22.0 -- not a known variable star
00:55:48.81 +44:10:48.4 -- not a known variable star
00:56:40.47 +48:44:11.4 -- a known variable star
00:56:54.71 +41:31:41.7 -- not a known variable star
00:57:04.39 +48:42:09.0 -- a known variable star
00:57:28.45 +42:47:54.3 -- a known variable star
00:58:20.83 +49:25:06.4 -- a known variable star
01:00:04.24 +48:40:23.8 -- a known variable star
01:00:20.71 +41:01:19.8 -- not a known variable star
01:00:21.25 +48:54:15.3 -- a known variable star
01:00:48.10 +50:23:41.6 -- a known variable star
01:02:24.96 +47:26:32.9 -- not a known variable star
01:03:40.80 +48:10:46.9 -- not a known variable star
01:05:51.98 +48:50:26.6 -- a known variable star
01:06:04.74 +49:51:20.0 -- not a known variable star
01:06:23.29 +47:20:01.6 -- a known variable star
01:07:07.67 +43:02:44.6 -- not a known variable star
01:07:26.54 +45:36:35.6 -- a known variable star
01:09:27.78 +42:40:17.6 -- not a known variable star
01:10:12.11 +50:22:50.0 -- a known variable star
01:10:12.93 +49:10:15.4 -- a known variable star
01:10:43.33 +43:20:57.2 -- not a known variable star
01:11:14.09 +50:23:29.3 -- a known variable star
01:11:45.37 +43:16:18.1 -- a known variable star
01:12:32.83 +50:51:24.3 -- a known variable star
01:13:46.30 +46:34:07.8 -- a known variable star
01:14:04.52 +47:52:07.5 -- a known variable star
01:14:22.06 +49:58:28.9 -- a known variable star
01:14:22.24 +47:04:47.6 -- a known variable star
01:15:42.26 +46:12:18.4 -- a known variable star
01:16:04.64 +50:11:40.0 -- a known variable star
01:16:19.81 +47:27:31.0 -- a known variable star
01:16:57.43 +49:34:43.7 -- a known variable star
01:17:29.78 +47:41:12.0 -- not a known variable star
01:17:55.72 +50:24:13.4 -- a known variable star
01:19:23.91 +48:26:38.1 -- not a known variable star
01:20:28.68 +43:52:02.2 -- not a known variable star
01:20:54.65 +49:35:51.8 -- not a known variable star
01:21:11.80 +48:29:08.2 -- not a known variable star
01:21:37.14 +43:32:51.2 -- a known variable star
01:22:04.52 +46:06:40.4 -- not a known variable star
01:23:44.46 +45:52:03.1 -- a known variable star
01:23:44.50 +49:24:07.3 -- not a known variable star
01:23:46.35 +47:16:25.4 -- not a known variable star
01:24:25.24 +45:36:20.1 -- a known variable star
01:25:48.53 +46:24:13.0 -- a known variable star
01:26:27.60 +49:53:58.1 -- a known variable star
01:26:55.54 +47:24:02.8 -- a known variable star
01:28:03.50 +49:29:53.6 -- a known variable star
01:28:47.66 +44:16:39.2 -- not a known variable star
01:29:26.69 +46:27:24.0 -- a known variable star
01:31:04.14 +47:34:41.3 -- a known variable star
01:31:54.80 +46:49:07.2 -- a known variable star
01:31:58.34 +45:46:20.7 -- a known variable star
01:33:35.62 +46:31:13.7 -- a known variable star
01:35:12.12 +46:33:47.6 -- not a known variable star
01:36:40.37 +42:51:19.4 -- a known variable star
01:37:29.69 +47:55:39.9 -- a known variable star
01:51:23.52 +49:56:14.5 -- not a known variable star
01:55:41.06 +50:00:11.6 -- not a known variable star
Found 398 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
480 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
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.65130784 -observatory 500
23:23:24.06 -01:59:21.3 Mercury (-0.1mag)
23:04:23.27 -07:30:18.7 Venus (-3.9mag)
21:42:45.67 -14:53:05.8 Mars (1.1mag)
07:06:06.25 +22:54:19.6 Jupiter (-2.5mag)
00:05:25.76 -01:44:30.8 Saturn (1.0mag)
03:39:59.43 +19:21:43.5 Uranus (5.7mag)
00:03:40.77 -01:01:38.2 Neptune (7.8mag)
20:29:06.93 -22:59:34.4 Pluto (14.5mag)
01:53:22.25 +16:09:43.3 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 22 02:38 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461093.65130784:
07:06:10.22 +22:54:14.4 Io (5.4mag)
07:06:17.71 +22:53:58.6 Europa (5.5mag)
07:05:56.91 +22:54:45.4 Ganymede (4.9mag)
07:06:25.21 +22:53:54.3 Callisto (6.2mag)
07:09:15.17 +23:10:42.8 Himalia (15.0mag)
07:06:07.47 +22:54:19.7 Thebe (15.9mag)
07:08:40.26 +23:19:11.1 Elara (17.0mag)
07:01:39.77 +24:02:18.2 Pasiphae (17.0mag)
07:15:07.15 +22:42:19.4 Carme (18.1mag)
00:05:37.45 -01:44:35.5 Titan (8.8mag)
00:05:31.22 -01:44:29.5 Rhea (10.1mag)
00:05:21.13 -01:45:51.8 Iapetus (11.5mag)
00:05:26.57 -01:44:33.9 Hyperion (14.8mag)
00:07:30.04 -01:31:30.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 22 02:38 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.65130784:
08:45:45.46 +24:30:42.7 JWST
11:33:29.99 +48:21:51.1 Chandra
15:21:47.26 -59:53:36.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 02:38 spacecraft.txt
############################################################
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)2461093.65130784 at 500
16:59:41.25 -11:03:49.1 17.5mag 10P/Tempel 2
03:37:18.56 +28:57:48.7 18.0mag 123P/West-Hartley
08:23:39.06 +60:42:57.6 18.4mag 124P/Mrkos
21:19:33.98 -07:38:50.3 22.1mag 141P/Machholz
01:21:08.52 +11:54:47.7 17.7mag 145P/Shoemaker-Levy 5
11:02:59.21 +30:34:31.0 17.9mag 164P/Christensen
09:33:08.07 -33:51:48.6 18.0mag 195P/Hill
15:52:03.25 -06:35:54.2 19.2mag 210P/Christensen
18:16:50.56 -21:28:31.4 17.3mag 218P/LINEAR
16:21:33.82 -18:10:56.6 15.2mag 235P/LINEAR
03:56:23.08 +27:44:28.7 17.8mag 240P/NEAT
15:17:37.58 +06:38:25.9 14.8mag 24P/Schaumasse
11:23:31.15 -03:23:09.9 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.89 +27:24:49.9 19.6mag 407P/PanSTARRS-Fuls
17:07:08.44 -11:19:14.3 17.6mag 40P/Vaisala 1
11:02:12.98 -08:51:53.5 16.6mag 43P/Wolf-Harrington
13:25:29.73 -05:49:38.6 20.0mag 489P/Denning
04:34:21.97 +48:34:34.8 17.8mag 493P/2024 Q2 (LONEOS)
06:04:23.11 +47:31:29.5 17.7mag 63P/Wild 1
23:14:36.17 -02:07:32.8 16.2mag 78P/Gehrels 2
20:01:29.65 -22:18:19.5 15.0mag 88P/Howell
15:27:54.59 -29:00:40.1 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.10 -72:35:54.8 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:50.01 +31:12:54.2 18.2mag C/2017 K2 (PanSTARRS)
20:06:38.17 -65:11:37.9 18.1mag C/2020 V2 (ZTF)
17:21:40.35 +04:21:22.1 16.3mag C/2021 G2 (ATLAS)
03:35:40.90 +24:36:42.1 15.8mag C/2022 N2 (PanSTARRS)
09:08:13.30 +29:49:33.9 15.3mag C/2022 QE78 (ATLAS)
08:35:40.59 -06:33:47.9 16.7mag C/2022 R6 (PanSTARRS)
23:53:02.02 +48:26:45.2 18.0mag C/2023 C2 (ATLAS)
09:51:07.95 -20:46:00.2 17.5mag C/2023 F3 (ATLAS)
20:34:45.07 +61:14:30.9 17.3mag C/2023 H5 (Lemmon)
19:34:30.12 -03:24:15.9 16.1mag C/2023 R1 (PANSTARRS)
02:48:55.25 +35:40:34.3 18.5mag C/2023 RS61 (PanSTARRS)
21:01:26.90 +81:19:56.4 18.0mag C/2023 X2 (Lemmon)
06:39:09.89 +63:49:13.3 17.3mag C/2024 A1 (ATLAS)
01:56:44.64 -24:37:56.8 11.2mag C/2024 E1 (Wierzchos)
11:44:58.76 -02:34:51.9 18.1mag C/2024 G2 (ATLAS)
19:28:18.91 +00:39:12.4 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.73 -01:42:53.4 17.7mag C/2024 G6 (ATLAS)
19:53:27.54 +03:15:06.0 15.6mag C/2024 J3 (ATLAS)
02:47:14.56 -31:34:29.6 15.4mag C/2024 T5 (ATLAS)
16:25:06.24 -58:13:47.2 15.6mag C/2025 A6 (Lemmon)
04:50:29.50 +62:14:32.3 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)
15:56:43.48 -13:01:19.6 14.8mag C/2025 L1 (ATLAS)
02:20:14.02 -19:05:57.6 16.7mag C/2025 Q3 (ATLAS)
02:09:34.43 +17:16:43.7 21.2mag C/2025 R2 (SWAN)
22:20:45.84 +17:39:14.6 16.4mag C/2025 R3 (PANSTARRS)
21:46:01.19 -16:50:24.4 21.5mag C/2025 T1 (ATLAS)
03:06:14.56 -20:34:03.4 18.3mag C/2026 A1 (MAPS)
21:03:01.76 +20:55:36.4 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 22 02:39 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
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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 22 02:38 tocp_transients_list.txt