This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.54 03:03:15.85 +02:54:13.0
174.75396 -46.27927 galactic Cet Second-epoch detections are separated by 1.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1074502033847168 | 03:03:15.48 +02:54:08.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 wl 1958PMcCO..13b....V AG+02 300
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 15.85 +02 54 13.0 11.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1074502033847168,2461093.6528,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1074502033847168 20260222.1528 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:15.85 +02:54:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.32 03:08:49.45 +10:59:39.3
168.69414 -39.37272 galactic Ari Second-epoch detections are separated by 5.8" 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 15590735580146304 | 03:08:50.05 +10:59:35.8 (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 22.1528* 03 08 49.45 +10 59 39.3 11.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15590735580146304,2461093.6528,11.32,0.05,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 15590735580146304 20260222.1528 11.32CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:49.45 +10:59:39.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.50 03:05:03.70 +01:54:25.8
176.23819 -46.66612 galactic Cet Second-epoch detections are separated by 3.7" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 674004923466624 | 03:05:04.44 +01:54:33.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1949TOYal..20.....B BD+01 535
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 05 03.70 +01 54 25.8 11.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 674004923466624,2461093.6528,11.50,0.05,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 674004923466624 20260222.1528 11.50CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:05:03.70 +01:54:25.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 01 59.53 +03 47 58.8 11.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BMAM-V877,2461093.6528,11.12,0.05,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
BMAM-V877 20260222.1528 11.12CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:59.53 +03:47:58.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 08 30.43 +10 26 48.3 10.9 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X Ari,2461093.6528,10.93,0.05,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
X Ari 20260222.1528 10.93CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:30.43 +10:26:48.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.66 03:02:29.86 +05:35:05.8
171.93123 -44.46389 galactic Cet Second-epoch detections are separated by 2.5" and 8.1 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 6902635215675520 | 03:02:30.44 +05:35:09.9 (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 22.1528* 03 02 29.86 +05 35 05.8 10.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6902635215675520,2461093.6528,10.66,0.05,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 6902635215675520 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:02:29.86 +05:35:05.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.20 03:03:01.41 +03:55:34.9
173.66899 -45.58627 galactic Cet Second-epoch detections are separated by 0.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1950331764866304 | 03:03:01.89 +03:55:41.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1949TOYal..20.....B BD+03 423
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 01.41 +03 55 34.9 10.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1950331764866304,2461093.6528,10.20,0.05,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 1950331764866304 20260222.1528 10.20CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:01.41 +03:55:34.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.38 02:55:44.35 +07:16:52.7
168.60028 -44.29291 galactic Cet Second-epoch detections are separated by 1.4" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8120550501719680 | 02:55:45.19 +07:16:52.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 44.35 +07 16 52.7 10.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8120550501719680,2461093.6528,10.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8120550501719680 20260222.1528 10.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:44.35 +07:16:52.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.45 02:55:31.51 +06:18:23.6
169.42834 -45.07159 galactic Cet Second-epoch detections are separated by 2.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7894085466178560 | 02:55:32.13 +06:18:25.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 31.51 +06 18 23.6 10.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7894085466178560,2461093.6528,10.45,0.05,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 7894085466178560 20260222.1528 10.45CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:31.51 +06:18:23.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.48 02:59:29.95 +06:20:18.8
170.44930 -44.40065 galactic Cet Second-epoch detections are separated by 4.8" and 8.1 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 7202389573123712 | 02:59:30.70 +06:20:22.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 29.95 +06 20 18.8 10.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7202389573123712,2461093.6528,10.48,0.05,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 7202389573123712 20260222.1528 10.48CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:29.95 +06:20:18.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.51 02:55:17.13 +08:08:18.0
167.72031 -43.70432 galactic Cet Second-epoch detections are separated by 1.3" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J043.8370+08.1431 | 02:55:18.25 +08:08:15.9 (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 22.1528* 02 55 17.13 +08 08 18.0 10.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J043.8370+08.1431,2461093.6528,10.51,0.05,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 J043.8370+08.1431 20260222.1528 10.51CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:17.13 +08:08:18.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.55 03:00:34.21 +10:48:04.6
166.81758 -40.81587 galactic Ari Second-epoch detections are separated by 1.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 27255454439256576 | 03:00:34.86 +10:47:58.3 (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 22.1528* 03 00 34.21 +10 48 04.6 10.6 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 27255454439256576,2461093.6528,10.55,0.05,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 27255454439256576 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:34.21 +10:48:04.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.59 02:58:12.40 +03:49:34.6
172.50669 -46.48208 galactic Cet Second-epoch detections are separated by 3.3" and 8.5 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 2086946084636800 | 02:58:12.75 +03:49:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 12.40 +03 49 34.6 10.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2086946084636800,2461093.6528,10.59,0.05,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 2086946084636800 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:12.40 +03:49:34.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.63 02:56:21.01 +06:33:59.0
169.41007 -44.74090 galactic Cet Second-epoch detections are separated by 2.9" and 8.6 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 7930266270668544 | 02:56:21.48 +06:33:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 21.01 +06 33 59.0 10.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7930266270668544,2461093.6528,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 7930266270668544 20260222.1528 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:21.01 +06:33:59.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.63 03:03:06.96 +10:06:04.1
168.04508 -40.96012 galactic Cet Second-epoch detections are separated by 1.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15054448783601408 | 03:03:07.88 +10:06:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1950TOYal..22.....B BD+09 388
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 06.96 +10 06 04.1 10.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15054448783601408,2461093.6528,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 15054448783601408 20260222.1528 10.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:06.96 +10:06:04.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.79 02:55:27.55 +06:57:40.4
168.81389 -44.58276 galactic Cet Second-epoch detections are separated by 6.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8093852985017984 | 02:55:28.22 +06:57:41.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 27.55 +06 57 40.4 10.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8093852985017984,2461093.6528,10.79,0.05,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 8093852985017984 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:27.55 +06:57:40.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 43 43.72 +06 55 30.5 10.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1083 Tau,2461093.6528,10.77,0.05,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
V1083 Tau 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:43.72 +06:55:30.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.81 02:57:55.29 +08:10:18.8
168.38385 -43.26286 galactic Cet Second-epoch detections are separated by 4.7" and 8.5 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 8742805363592576 | 02:57:55.95 +08:10:17.4 (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 22.1528* 02 57 55.29 +08 10 18.8 10.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8742805363592576,2461093.6528,10.81,0.05,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 8742805363592576 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:55.29 +08:10:18.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.84 02:59:59.96 +07:06:07.6
169.88030 -43.74390 galactic Cet Second-epoch detections are separated by 1.4" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7316670062908288 | 03:00:00.65 +07:06:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1950TOYal..22.....B BD+06 463
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 59.96 +07 06 07.6 10.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7316670062908288,2461093.6528,10.84,0.05,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 7316670062908288 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:59.96 +07:06:07.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.91 02:56:37.16 +01:45:05.7
174.18512 -48.26250 galactic Cet Second-epoch detections are separated by 3.1" and 8.2 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 1171705733851136 | 02:56:37.64 +01:45:10.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A2 1949TOYal..20.....B BD+01 514
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 37.16 +01 45 05.7 10.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1171705733851136,2461093.6528,10.91,0.05,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
Gaia DR3 1171705733851136 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:37.16 +01:45:05.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.93 02:57:00.74 +05:31:44.8
170.54846 -45.41685 galactic Cet Second-epoch detections are separated by 5.3" and 9.0 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 7042032674251136 | 02:57:01.07 +05:31:48.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1949TOYal..20.....B BD+04 470
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 00.74 +05 31 44.8 10.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7042032674251136,2461093.6528,10.93,0.05,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 7042032674251136 20260222.1528 10.93CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:00.74 +05:31:44.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.12 02:57:54.12 +07:26:05.2
169.03342 -43.83004 galactic Cet Second-epoch detections are separated by 8.5" and 9.4 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 8138142687785472 | 02:57:54.65 +07:26:06.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 54.12 +07 26 05.2 11.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8138142687785472,2461093.6528,11.12,0.05,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 8138142687785472 20260222.1528 11.12CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:54.12 +07:26:05.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.15 02:56:18.34 +09:18:07.9
166.98296 -42.64178 galactic Cet Second-epoch detections are separated by 0.8" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 20992838070186240 | 02:56:19.18 +09:18:03.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG+09 273
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 18.34 +09 18 07.9 11.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20992838070186240,2461093.6528,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 20992838070186240 20260222.1528 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:18.34 +09:18:07.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.27 03:01:24.55 +07:10:56.7
170.17151 -43.45359 galactic Cet Second-epoch detections are separated by 5.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7684834659506688 | 03:01:25.36 +07:10:57.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1950TOYal..22.....B BD+06 464
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 24.55 +07 10 56.7 11.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7684834659506688,2461093.6528,11.27,0.05,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 7684834659506688 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:24.55 +07:10:56.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.24 02:57:29.66 +02:53:42.5
173.24622 -47.28405 galactic Cet Second-epoch detections are separated by 0.9" and 8.1 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 1402912413121792 | 02:57:30.04 +02:53:45.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A0 1958PMcCO..13b....V AG+02 290
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 29.66 +02 53 42.5 11.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1402912413121792,2461093.6528,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1402912413121792 20260222.1528 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:29.66 +02:53:42.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.40 02:57:22.15 +05:20:42.6
170.81692 -45.49598 galactic Cet Second-epoch detections are separated by 0.5" and 8.0 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 6848862225009664 | 02:57:22.57 +05:20:43.7 (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 22.1528* 02 57 22.15 +05 20 42.6 11.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6848862225009664,2461093.6528,11.40,0.05,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 6848862225009664 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:22.15 +05:20:42.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.41 02:55:57.77 +04:06:13.8
171.63349 -46.65479 galactic Cet Second-epoch detections are separated by 2.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5109091232499968 | 02:55:58.22 +04:06:24.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 57.77 +04 06 13.8 11.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5109091232499968,2461093.6528,11.41,0.05,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 5109091232499968 20260222.1528 11.41CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:57.77 +04:06:13.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.41 02:59:10.44 +08:56:21.6
168.03901 -42.47484 galactic Cet Second-epoch detections are separated by 0.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8947550749328000 | 02:59:11.03 +08:56:18.9 (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 22.1528* 02 59 10.44 +08 56 21.6 11.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8947550749328000,2461093.6528,11.41,0.05,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 8947550749328000 20260222.1528 11.41CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:10.44 +08:56:21.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.40 02:55:25.57 +06:20:17.5
169.37277 -45.06349 galactic Cet Second-epoch detections are separated by 1.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7894463423299840 | 02:55:25.99 +06:20:20.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1958PMcCO..13b....V AG+06 302
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 25.57 +06 20 17.5 11.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7894463423299840,2461093.6528,11.40,0.05,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 7894463423299840 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:25.57 +06:20:17.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.38 03:03:53.64 +09:45:11.1
168.53624 -41.10356 galactic Cet Second-epoch detections are separated by 4.4" and 8.4 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 14985037816540928 | 03:03:54.46 +09:45:11.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 1958PMcCO..13b....V AG+09 280
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 53.64 +09 45 11.1 11.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 14985037816540928,2461093.6528,11.38,0.05,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 14985037816540928 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:53.64 +09:45:11.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.46 02:56:14.93 +09:21:05.1
166.92618 -42.61221 galactic Cet Second-epoch detections are separated by 0.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 20995247547587328 | 02:56:15.80 +09:21:00.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG+09 272
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 14.93 +09 21 05.1 11.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20995247547587328,2461093.6528,11.46,0.05,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 20995247547587328 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:14.93 +09:21:05.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 29 25.82 +06 19 09.0 10.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J032926+0619.1,2461093.6528,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J032926+0619.1 20260222.1528 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:29:25.82 +06:19:09.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 23 43.97 +03 53 23.5 9.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J032344+0353.3,2461093.6528,8.97,0.05,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
ASAS J032344+0353.3 20260222.1528 8.97CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:43.97 +03:53:23.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 23 35.75 +09 23 52.0 11.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J032336+0923.9,2461093.6528,11.30,0.05,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
ASAS J032336+0923.9 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:23:35.75 +09:23:52.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.70 03:00:12.62 +02:02:10.0
174.84712 -47.43264 galactic Cet Second-epoch detections are separated by 4.7" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 535359083634944 | 03:00:12.34 +02:02:04.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 12.62 +02 02 10.0 13.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 535359083634944,2461093.6528,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 535359083634944 20260222.1528 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:12.62 +02:02:10.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.76 03:02:33.29 +02:04:40.8
175.41640 -46.99070 galactic Cet Second-epoch detections are separated by 6.6" and 8.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:02:33.29 +02:04:40.8 (user input) | T | P | (position from user input) 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 22.1528* 03 02 33.29 +02 04 40.8 13.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:02:33.29 +02:04:40.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.62 03:03:32.99 +08:44:02.0
169.33289 -41.93434 galactic Cet Second-epoch detections are separated by 0.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:03:32.99 +08:44:02.0 (user input) | T | P | (position from user input) 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 22.1528* 03 03 32.99 +08 44 02.0 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:32.99 +08:44:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.55 02:59:27.39 +06:31:39.1
170.26392 -44.26560 galactic Cet Second-epoch detections are separated by 2.5" and 8.1 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 J044.8572+06.5319 | 02:59:27.74 +06:31:34.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 27.39 +06 31 39.1 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J044.8572+06.5319,2461093.6528,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J044.8572+06.5319 20260222.1528 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:27.39 +06:31:39.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.46 02:59:30.72 +01:43:01.3
174.99474 -47.78243 galactic Cet Second-epoch detections are separated by 5.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 502137512125056 | 02:59:30.83 +01:43:07.3 (Gaia DR3) | T | P | 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 22.1528* 02 59 30.72 +01 43 01.3 13.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 502137512125056,2461093.6528,13.46,0.05,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 502137512125056 20260222.1528 13.46CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:30.72 +01:43:01.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 08 54.76 +09 51 45.2 13.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:54.76 +09:51:45.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.38 02:59:16.27 +01:38:11.8
175.01506 -47.88195 galactic Cet Second-epoch detections are separated by 1.7" and 8.5 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 448566384512512 | 02:59:16.28 +01:38:03.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 16.27 +01 38 11.8 13.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 448566384512512,2461093.6528,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 448566384512512 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:16.27 +01:38:11.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.42 03:13:33.62 +07:37:43.3
172.77877 -41.09682 galactic Cet Second-epoch detections are separated by 5.3" and 8.0 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 | 03:13:33.62 +07:37:43.3 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 13 33.62 +07 37 43.3 13.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:33.62 +07:37:43.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.29 03:00:36.42 +02:50:13.1
174.13040 -46.78978 galactic Cet Second-epoch detections are separated by 2.0" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1718197372427264 | 03:00:36.21 +02:50:06.6 (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 22.1528* 03 00 36.42 +02 50 13.1 13.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1718197372427264,2461093.6528,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1718197372427264 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:36.42 +02:50:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.32 03:07:08.61 +01:29:33.2
177.19881 -46.58083 galactic Cet Second-epoch detections are separated by 5.6" and 9.0 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 3267209011074300928 | 03:07:07.93 +01:29:35.6 (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 22.1528* 03 07 08.61 +01 29 33.2 13.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3267209011074300928,2461093.6528,13.32,0.05,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 3267209011074300928 20260222.1528 13.32CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:08.61 +01:29:33.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.17 02:56:45.33 +05:17:06.0
170.71040 -45.64225 galactic Cet Second-epoch detections are separated by 4.4" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5345653735562368 | 02:56:44.86 +05:17:07.5 (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 22.1528* 02 56 45.33 +05 17 06.0 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5345653735562368,2461093.6528,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5345653735562368 20260222.1528 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:45.33 +05:17:06.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.11 02:56:19.85 +03:40:48.2
172.14902 -46.90655 galactic Cet Second-epoch detections are separated by 3.9" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2057637227790592 | 02:56:21.29 +03:40:51.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 19.85 +03 40 48.2 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2057637227790592,2461093.6528,13.11,0.05,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 2057637227790592 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:19.85 +03:40:48.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.51 03:36:19.38 +04:35:45.8
180.76008 -39.10414 galactic Tau Second-epoch detections are separated by 4.0" 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 | target | 03:36:19.38 +04:35:45.8 (user input) | T | P | (position from user input) SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 36 19.38 +04 35 45.8 13.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:19.38 +04:35:45.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.13 02:58:42.40 +05:34:33.7
170.95289 -45.10235 galactic Cet Second-epoch detections are separated by 6.4" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6858998347843072 | 02:58:41.97 +05:34:32.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 42.40 +05 34 33.7 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6858998347843072,2461093.6528,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 6858998347843072 20260222.1528 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:42.40 +05:34:33.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.11 03:01:43.48 +09:24:11.1
168.29082 -41.71560 galactic Cet Second-epoch detections are separated by 2.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 14991055066307840 | 03:01:43.87 +09:24:05.9 (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 22.1528* 03 01 43.48 +09 24 11.1 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 14991055066307840,2461093.6528,13.11,0.05,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 14991055066307840 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:43.48 +09:24:11.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.87 02:59:43.92 +08:44:48.3
168.34985 -42.53466 galactic Cet Second-epoch detections are separated by 1.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8894228730549248 | 02:59:44.42 +08:44:46.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 43.92 +08 44 48.3 12.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8894228730549248,2461093.6528,12.87,0.05,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 8894228730549248 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:43.92 +08:44:48.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.12 03:09:08.33 +10:57:07.6
168.80548 -39.35453 galactic Ari Second-epoch detections are separated by 3.1" and 8.0 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 15542662010877952 | 03:09:08.80 +10:57:04.5 (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 22.1528* 03 09 08.33 +10 57 07.6 13.1 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15542662010877952,2461093.6528,13.12,0.05,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 15542662010877952 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:09:08.33 +10:57:07.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.10 03:09:53.66 +10:01:58.2
169.76963 -39.92755 galactic Cet Second-epoch detections are separated by 4.5" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15272117726206336 | 03:09:53.17 +10:01:57.6 (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 22.1528* 03 09 53.66 +10 01 58.2 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15272117726206336,2461093.6528,13.10,0.05,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 15272117726206336 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:09:53.66 +10:01:58.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.97 03:03:06.80 +02:01:27.9
175.61645 -46.92988 galactic Cet Second-epoch detections are separated by 3.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 851816569480576 | 03:03:06.43 +02:01:22.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 06.80 +02 01 27.9 13.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 851816569480576,2461093.6528,12.97,0.05,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 851816569480576 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:06.80 +02:01:27.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.71 03:01:46.89 +09:56:00.0
167.85207 -41.29918 galactic Cet Second-epoch detections are separated by 5.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15047576835907072 | 03:01:46.37 +09:56:03.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 46.89 +09 56 00.0 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15047576835907072,2461093.6528,12.71,0.05,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 15047576835907072 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:46.89 +09:56:00.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.65 02:58:55.18 +03:00:13.0
173.51664 -46.96071 galactic Cet Second-epoch detections are separated by 5.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1774135026457216 | 02:58:54.51 +03:00:08.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 55.18 +03 00 13.0 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1774135026457216,2461093.6528,12.65,0.05,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 1774135026457216 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:55.18 +03:00:13.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.63 02:58:01.54 +03:47:53.2
172.48631 -46.53341 galactic Cet Second-epoch detections are separated by 6.5" and 8.1 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 2085498680532224 | 02:58:01.11 +03:47:50.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 01.54 +03 47 53.2 12.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2085498680532224,2461093.6528,12.63,0.05,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 2085498680532224 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:01.54 +03:47:53.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.68 03:05:24.21 +08:21:19.0
170.13163 -41.91943 galactic Cet Second-epoch detections are separated by 5.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 8631342371843840 | 03:05:24.80 +08:21:15.7 (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 22.1528* 03 05 24.21 +08 21 19.0 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 8631342371843840,2461093.6528,12.68,0.05,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
Large-amplitude variable Gaia DR2 8631342371843840 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:05:24.21 +08:21:19.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.54 02:58:51.62 +05:04:53.6
171.46214 -45.44519 galactic Cet Second-epoch detections are separated by 3.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6778733999246336 | 02:58:51.21 +05:04:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 51.62 +05 04 53.6 12.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6778733999246336,2461093.6528,12.54,0.05,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 6778733999246336 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:51.62 +05:04:53.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.36 03:00:02.07 +02:56:08.1
173.88002 -46.81780 galactic Cet Second-epoch detections are separated by 8.9" 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 1723518836561280 | 03:00:01.51 +02:56:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 02.07 +02 56 08.1 12.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1723518836561280,2461093.6528,12.36,0.05,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 1723518836561280 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:02.07 +02:56:08.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.30 03:03:54.16 +05:14:27.1
172.61836 -44.47960 galactic Cet Second-epoch detections are separated by 0.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3876366899115904 | 03:03:54.77 +05:14:28.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 54.16 +05 14 27.1 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3876366899115904,2461093.6528,12.30,0.05,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 3876366899115904 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:54.16 +05:14:27.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.07 03:03:51.10 +03:51:53.7
173.94258 -45.48768 galactic Cet Second-epoch detections are separated by 1.0" and 8.1 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 1946655272858496 | 03:03:51.60 +03:51:59.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 51.10 +03 51 53.7 12.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1946655272858496,2461093.6528,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1946655272858496 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:51.10 +03:51:53.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.96 02:58:13.23 +04:21:34.0
171.98835 -46.08715 galactic Cet Second-epoch detections are separated by 2.8" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2213969741771008 | 02:58:12.67 +04:21:31.4 (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 22.1528* 02 58 13.23 +04 21 34.0 12.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2213969741771008,2461093.6528,11.96,0.05,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 2213969741771008 20260222.1528 11.96CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:13.23 +04:21:34.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.55 03:03:34.41 +07:25:33.1
170.50360 -42.91631 galactic Cet Second-epoch detections are separated by 3.5" and 8.5 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 7715861503232384 | 03:03:34.90 +07:25:32.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 34.41 +07 25 33.1 11.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7715861503232384,2461093.6528,11.55,0.05,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 7715861503232384 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:34.41 +07:25:33.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.26 03:04:00.64 +09:39:57.9
168.63997 -41.15142 galactic Cet Second-epoch detections are separated by 3.9" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 14981159461673984 | 03:04:01.05 +09:39:54.9 (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 22.1528* 03 04 00.64 +09 39 57.9 10.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 14981159461673984,2461093.6528,10.26,0.05,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 14981159461673984 20260222.1528 10.26CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:04:00.64 +09:39:57.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.69 03:00:20.03 +01:24:56.7
175.52792 -47.85145 galactic Cet Second-epoch detections are separated by 4.0" and 8.8 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 429531089342464 | 03:00:20.37 +01:25:01.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG+01 306
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 20.03 +01 24 56.7 10.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 429531089342464,2461093.6528,10.69,0.05,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 429531089342464 20260222.1528 10.69CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:20.03 +01:24:56.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.77 02:57:54.79 +08:10:19.7
168.38145 -43.26399 galactic Cet Second-epoch detections are separated by 1.9" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8742805363592576 | 02:57:55.95 +08:10:17.4 (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 22.1528* 02 57 54.79 +08 10 19.7 10.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8742805363592576,2461093.6528,10.77,0.05,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 8742805363592576 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:54.79 +08:10:19.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.83 03:02:41.61 +07:04:00.7
170.60567 -43.32978 galactic Cet Second-epoch detections are separated by 1.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7633157612463232 | 03:02:42.45 +07:04:00.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1950TOYal..22.....B BD+06 467
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 02 41.61 +07 04 00.7 10.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7633157612463232,2461093.6528,10.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 7633157612463232 20260222.1528 10.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:02:41.61 +07:04:00.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.85 03:01:26.74 +02:07:53.8
175.07230 -47.14796 galactic Cet Second-epoch detections are separated by 1.3" and 8.0 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 J045.3673+02.1398 | 03:01:27.14 +02:08:00.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 26.74 +02 07 53.8 10.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J045.3673+02.1398,2461093.6528,10.85,0.05,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
ATO J045.3673+02.1398 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:26.74 +02:07:53.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 10.95 03:02:10.03 +07:51:21.4
169.75930 -42.82236 galactic Cet Second-epoch detections are separated by 1.4" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8495724484999168 | 03:02:10.73 +07:51:20.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1950TOYal..22.....B BD+07 465
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 02 10.03 +07 51 21.4 10.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8495724484999168,2461093.6528,10.95,0.05,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
Gaia DR3 8495724484999168 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:02:10.03 +07:51:21.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.02 02:58:13.45 +03:10:02.9
173.16684 -46.96087 galactic Cet Second-epoch detections are separated by 3.8" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1791761572209792 | 02:58:13.77 +03:10:08.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG+02 292
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 13.45 +03 10 02.9 11.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1791761572209792,2461093.6528,11.02,0.05,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 1791761572209792 20260222.1528 11.02CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:13.45 +03:10:02.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.05 03:01:45.83 +07:16:41.8
170.17570 -43.32353 galactic Cet Second-epoch detections are separated by 2.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7698819073017600 | 03:01:46.56 +07:16:40.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 45.83 +07 16 41.8 11.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7698819073017600,2461093.6528,11.05,0.05,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 7698819073017600 20260222.1528 11.05CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:45.83 +07:16:41.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.06 02:57:10.21 +08:34:18.4
167.83782 -43.07353 galactic Cet Second-epoch detections are separated by 1.0" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8837977543281536 | 02:57:10.68 +08:34:16.7 (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 22.1528* 02 57 10.21 +08 34 18.4 11.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8837977543281536,2461093.6528,11.06,0.05,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 8837977543281536 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:10.21 +08:34:18.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.19 03:09:22.26 +10:48:44.2
168.97930 -39.42348 galactic Ari Second-epoch detections are separated by 4.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15537409266205824 | 03:09:22.79 +10:48:35.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1958PMcCO..13b....V AG+10 335
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 09 22.26 +10 48 44.2 11.2 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15537409266205824,2461093.6528,11.19,0.05,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 15537409266205824 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:09:22.26 +10:48:44.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.14 02:57:44.32 +06:54:45.2
169.46179 -44.25376 galactic Cet Second-epoch detections are separated by 3.1" and 8.1 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 8037777892070272 | 02:57:45.16 +06:54:47.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 44.32 +06 54 45.2 11.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8037777892070272,2461093.6528,11.14,0.05,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 8037777892070272 20260222.1528 11.14CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:44.32 +06:54:45.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.18 02:56:14.59 +03:29:04.4
172.31914 -47.06539 galactic Cet Second-epoch detections are separated by 5.5" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2050662200940544 | 02:56:15.19 +03:29:09.1 (Gaia DR3) | T | P | 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 22.1528* 02 56 14.59 +03 29 04.4 11.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2050662200940544,2461093.6528,11.18,0.05,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 2050662200940544 20260222.1528 11.18CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:14.59 +03:29:04.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.31 03:08:49.16 +10:59:45.0
168.69165 -39.37228 galactic Ari Second-epoch detections are separated by 1.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15590735580146304 | 03:08:50.05 +10:59:35.8 (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 22.1528* 03 08 49.16 +10 59 45.0 11.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15590735580146304,2461093.6528,11.31,0.05,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 15590735580146304 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:49.16 +10:59:45.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 00 26.59 +02 10 54.9 11.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J030027+0211.0,2461093.6528,11.29,0.05,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
ASAS J030027+0211.0 20260222.1528 11.29CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:26.59 +02:10:54.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.29 02:55:44.79 +04:39:46.4
171.03342 -46.27451 galactic Cet Second-epoch detections are separated by 3.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5284566416253568 | 02:55:45.10 +04:39:51.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949TOYal..20.....B BD+04 465
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 44.79 +04 39 46.4 11.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5284566416253568,2461093.6528,11.29,0.05,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 5284566416253568 20260222.1528 11.29CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:44.79 +04:39:46.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.34 03:04:50.92 +08:23:38.9
169.95842 -41.98066 galactic Cet Second-epoch detections are separated by 3.6" and 8.2 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 8634159870901120 | 03:04:51.73 +08:23:39.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 wl 1958PMcCO..13b....V AG+08 325
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 04 50.92 +08 23 38.9 11.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8634159870901120,2461093.6528,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8634159870901120 20260222.1528 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:04:50.92 +08:23:38.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.31 02:54:33.08 +02:36:46.1
172.73597 -47.99228 galactic Cet Second-epoch detections are separated by 1.2" and 8.2 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 1555675809991936 | 02:54:33.43 +02:36:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949TOYal..20.....B BD+02 446
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 54 33.08 +02 36 46.1 11.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1555675809991936,2461093.6528,11.31,0.05,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 1555675809991936 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:54:33.08 +02:36:46.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.33 03:01:50.71 +07:44:29.8
169.77932 -42.96098 galactic Cet Second-epoch detections are separated by 1.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8492769547504256 | 03:01:51.46 +07:44:30.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 50.71 +07 44 29.8 11.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8492769547504256,2461093.6528,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8492769547504256 20260222.1528 11.33CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:50.71 +07:44:29.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.30 03:00:38.54 +02:34:32.9
174.40549 -46.97124 galactic Cet Second-epoch detections are separated by 7.9" and 9.0 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 1697959486536320 | 03:00:38.97 +02:34:40.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 38.54 +02 34 32.9 11.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1697959486536320,2461093.6528,11.30,0.05,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 1697959486536320 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:38.54 +02:34:32.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.35 03:07:24.85 +10:40:47.5
168.61693 -39.83658 galactic Ari Second-epoch detections are separated by 3.1" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15555379409552896 | 03:07:25.39 +10:40:42.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 1958PMcCO..13b....V AG+10 331
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 07 24.85 +10 40 47.5 11.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15555379409552896,2461093.6528,11.35,0.05,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 15555379409552896 20260222.1528 11.35CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:24.85 +10:40:47.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.38 02:55:58.76 +06:07:28.3
169.71761 -45.13630 galactic Cet Second-epoch detections are separated by 4.3" 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 | Gaia DR3 7137140430003712 | 02:55:59.48 +06:07:30.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1958PMcCO..13b....V AG+05 307
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 58.76 +06 07 28.3 11.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7137140430003712,2461093.6528,11.38,0.05,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 7137140430003712 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:58.76 +06:07:28.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.44 03:05:38.22 +10:39:28.4
168.20032 -40.13527 galactic Ari Second-epoch detections are separated by 4.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15194494781621632 | 03:05:38.92 +10:39:25.1 (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 22.1528* 03 05 38.22 +10 39 28.4 11.4 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15194494781621632,2461093.6528,11.44,0.05,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 15194494781621632 20260222.1528 11.44CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:05:38.22 +10:39:28.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.43 02:59:40.18 +02:17:19.5
174.44359 -47.34641 galactic Cet Second-epoch detections are separated by 2.3" and 8.5 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 560647851057152 | 02:59:40.54 +02:17:23.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG+02 293
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 40.18 +02 17 19.5 11.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 560647851057152,2461093.6528,11.43,0.05,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 560647851057152 20260222.1528 11.43CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:40.18 +02:17:19.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.41 02:58:59.80 +07:18:50.7
169.42798 -43.74580 galactic Cet Second-epoch detections are separated by 2.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8086259482884864 | 02:59:00.84 +07:18:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 59.80 +07 18 50.7 11.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8086259482884864,2461093.6528,11.41,0.05,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 8086259482884864 20260222.1528 11.41CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:59.80 +07:18:50.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.48 02:59:21.12 +01:44:14.1
174.93123 -47.79610 galactic Cet Second-epoch detections are separated by 0.6" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 503065225060864 | 02:59:21.40 +01:44:26.1 (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 22.1528* 02 59 21.12 +01 44 14.1 11.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 503065225060864,2461093.6528,11.48,0.05,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 503065225060864 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:21.12 +01:44:14.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.53 03:03:23.85 +08:38:29.7
169.37549 -42.02887 galactic Cet Second-epoch detections are separated by 5.1" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8701264440090240 | 03:03:24.79 +08:38:26.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 23.85 +08 38 29.7 11.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8701264440090240,2461093.6528,11.53,0.05,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 8701264440090240 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:23.85 +08:38:29.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.53 02:58:04.98 +07:34:12.7
168.95961 -43.69772 galactic Cet Second-epoch detections are separated by 7.0" and 8.8 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 8143983843299328 | 02:58:05.72 +07:34:11.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 04.98 +07 34 12.7 11.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8143983843299328,2461093.6528,11.53,0.05,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 8143983843299328 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:04.98 +07:34:12.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.52 02:59:09.94 +08:56:18.7
168.03756 -42.47677 galactic Cet Second-epoch detections are separated by 3.0" and 8.1 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 8947550749328000 | 02:59:11.03 +08:56:18.9 (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 22.1528* 02 59 09.94 +08 56 18.7 11.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8947550749328000,2461093.6528,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8947550749328000 20260222.1528 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:09.94 +08:56:18.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.51 02:56:33.58 +03:47:53.5
172.09400 -46.78086 galactic Cet Second-epoch detections are separated by 8.8" and 9.1 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 2094299068625920 | 02:56:33.93 +03:47:57.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 33.58 +03 47 53.5 11.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2094299068625920,2461093.6528,11.51,0.05,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 2094299068625920 20260222.1528 11.51CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:33.58 +03:47:53.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.63 02:59:41.13 +04:05:57.7
172.62946 -46.03108 galactic Cet Second-epoch detections are separated by 4.0" and 8.5 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 2145495079120896 | 02:59:41.50 +04:06:01.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 1958PMcCO..13b....V AG+03 342
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 41.13 +04 05 57.7 11.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2145495079120896,2461093.6528,11.63,0.05,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 2145495079120896 20260222.1528 11.63CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:41.13 +04:05:57.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.59 02:56:14.34 +03:34:42.2
172.22490 -46.99699 galactic Cet Second-epoch detections are separated by 6.5" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2054746714162560 | 02:56:14.96 +03:34:47.1 (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) 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 22.1528* 02 56 14.34 +03 34 42.2 11.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2054746714162560,2461093.6528,11.59,0.05,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
Large-amplitude variable Gaia DR2 2054746714162560 20260222.1528 11.59CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:14.34 +03:34:42.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 56 42.32 +06 42 12.7 11.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8026817135505280,2461093.6528,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8026817135505280 20260222.1528 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:42.32 +06:42:12.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.65 02:58:00.37 +10:14:03.0
166.63681 -41.65272 galactic Cet Second-epoch detections are separated by 1.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 27116327562916096 | 02:57:59.91 +10:14:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 00.37 +10 14 03.0 11.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 27116327562916096,2461093.6528,11.65,0.05,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 27116327562916096 20260222.1528 11.65CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:00.37 +10:14:03.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 02 25.30 +08 25 00.4 11.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,11.63,0.05,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
VARIABLE_NAME 20260222.1528 11.63CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:02:25.30 +08:25:00.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.71 03:01:46.00 +09:26:34.2
168.26729 -41.67847 galactic Cet Second-epoch detections are separated by 2.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 14991639181858304 | 03:01:46.70 +09:26:35.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F8 1958PMcCO..13b....V AG+09 278 J-Ks=1.512+/- (Very red! L if it's a dwarf)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 46.00 +09 26 34.2 11.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 14991639181858304,2461093.6528,11.71,0.05,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 14991639181858304 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:46.00 +09:26:34.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.75 03:01:54.94 +08:42:56.5
168.93537 -42.21061 galactic Cet Second-epoch detections are separated by 3.7" and 8.0 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 8713595290388608 | 03:01:56.00 +08:42:55.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 54.94 +08 42 56.5 11.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8713595290388608,2461093.6528,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8713595290388608 20260222.1528 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:54.94 +08:42:56.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.78 03:01:12.43 +03:59:49.7
173.12843 -45.84659 galactic Cet Second-epoch detections are separated by 1.9" and 8.1 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 2150816542672256 | 03:01:12.87 +03:59:52.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 12.43 +03 59 49.7 11.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2150816542672256,2461093.6528,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2150816542672256 20260222.1528 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:12.43 +03:59:49.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 57 38.17 +07 10 43.2 11.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KO Cet,2461093.6528,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KO Cet 20260222.1528 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:38.17 +07:10:43.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.88 02:59:57.50 +07:58:29.0
169.08671 -43.08870 galactic Cet Second-epoch detections are separated by 5.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8556708725234688 | 02:59:58.47 +07:58:29.9 (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 22.1528* 02 59 57.50 +07 58 29.0 11.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8556708725234688,2461093.6528,11.88,0.05,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 8556708725234688 20260222.1528 11.88CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:57.50 +07:58:29.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.93 03:00:03.90 +06:07:39.1
170.79255 -44.46571 galactic Cet Second-epoch detections are separated by 4.3" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7181189614590080 | 03:00:04.91 +06:07:39.4 (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 22.1528* 03 00 03.90 +06 07 39.1 11.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7181189614590080,2461093.6528,11.93,0.05,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 7181189614590080 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:03.90 +06:07:39.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.82 02:56:19.99 +04:20:15.9
171.50539 -46.41926 galactic Cet Second-epoch detections are separated by 3.0" and 8.0 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 5131287623478400 | 02:56:20.28 +04:20:26.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 19.99 +04 20 15.9 11.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5131287623478400,2461093.6528,11.82,0.05,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 5131287623478400 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:19.99 +04:20:15.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.97 03:01:53.16 +08:37:34.2
169.00620 -42.28355 galactic Cet Second-epoch detections are separated by 6.0" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8709716935518080 | 03:01:54.12 +08:37:31.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 53.16 +08 37 34.2 12.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8709716935518080,2461093.6528,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8709716935518080 20260222.1528 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:53.16 +08:37:34.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.87 02:56:15.97 +05:56:08.4
169.96931 -45.23264 galactic Cet Second-epoch detections are separated by 3.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7120613395855488 | 02:56:16.71 +05:56:13.1 (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 22.1528* 02 56 15.97 +05 56 08.4 11.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7120613395855488,2461093.6528,11.87,0.05,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 7120613395855488 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:15.97 +05:56:08.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.90 03:07:00.94 +09:59:55.2
169.09857 -40.41797 galactic Cet Second-epoch detections are separated by 4.9" and 8.4 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 15095852268404480 | 03:07:01.55 +09:59:51.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 07 00.94 +09 59 55.2 11.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15095852268404480,2461093.6528,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 15095852268404480 20260222.1528 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:00.94 +09:59:55.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.89 02:54:43.18 +06:06:52.2
169.38915 -45.34763 galactic Cet Second-epoch detections are separated by 3.8" and 8.4 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 7884018062842752 | 02:54:43.71 +06:06:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 54 43.18 +06 06 52.2 11.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7884018062842752,2461093.6528,11.89,0.05,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 7884018062842752 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:54:43.18 +06:06:52.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.97 02:59:38.01 +04:18:36.6
172.40973 -45.88522 galactic Cet Second-epoch detections are separated by 1.3" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2221430100907776 | 02:59:38.62 +04:18:38.5 (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 22.1528* 02 59 38.01 +04 18 36.6 12.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2221430100907776,2461093.6528,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2221430100907776 20260222.1528 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:38.01 +04:18:36.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.03 03:01:09.19 +08:51:04.5
168.62295 -42.22887 galactic Cet Second-epoch detections are separated by 2.7" and 8.2 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 8906976193506432 | 03:01:09.82 +08:51:06.7 (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 22.1528* 03 01 09.19 +08 51 04.5 12.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8906976193506432,2461093.6528,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8906976193506432 20260222.1528 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:09.19 +08:51:04.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.04 03:01:49.27 +01:45:00.7
175.56664 -47.35212 galactic Cet Second-epoch detections are separated by 1.6" and 8.1 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 470801430790272 | 03:01:49.48 +01:45:06.7 (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 22.1528* 03 01 49.27 +01 45 00.7 12.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 470801430790272,2461093.6528,12.04,0.05,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 470801430790272 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:49.27 +01:45:00.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.95 02:56:58.22 +10:28:48.8
166.16512 -41.61869 galactic Ari Second-epoch detections are separated by 7.5" 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 27323486721297408 | 02:56:58.79 +10:28:49.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 58.22 +10 28 48.8 11.9 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 27323486721297408,2461093.6528,11.95,0.05,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 27323486721297408 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:58.22 +10:28:48.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.99 03:01:26.91 +07:51:39.4
169.57115 -42.93501 galactic Cet Second-epoch detections are separated by 5.9" and 8.8 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 8506715305911424 | 03:01:27.49 +07:51:40.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G4 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 26.91 +07 51 39.4 12.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8506715305911424,2461093.6528,11.99,0.05,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 8506715305911424 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:26.91 +07:51:39.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 11.99 02:56:03.69 +08:45:06.3
167.39135 -43.10767 galactic Cet Second-epoch detections are separated by 1.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 20865024139209216 | 02:56:04.20 +08:45:03.2 (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 22.1528* 02 56 03.69 +08 45 06.3 12.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20865024139209216,2461093.6528,11.99,0.05,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 20865024139209216 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:03.69 +08:45:06.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 01 39.22 +10 56 36.6 12.1 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 27262532545349888,2461093.6528,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 27262532545349888 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:39.22 +10:56:36.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.05 03:05:58.16 +10:47:15.0
168.17303 -39.98353 galactic Ari Second-epoch detections are separated by 5.3" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15573899308528768 | 03:05:58.96 +10:47:10.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 05 58.16 +10 47 15.0 12.1 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15573899308528768,2461093.6528,12.05,0.05,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 15573899308528768 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:05:58.16 +10:47:15.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.07 02:57:41.86 +06:06:30.2
170.18910 -44.86879 galactic Cet Second-epoch detections are separated by 8.2" and 9.3 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 7145245032580480 | 02:57:42.29 +06:06:33.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 41.86 +06 06 30.2 12.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7145245032580480,2461093.6528,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 7145245032580480 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:41.86 +06:06:30.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.02 02:55:52.85 +08:44:58.6
167.34572 -43.13747 galactic Cet Second-epoch detections are separated by 3.3" and 8.1 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 20864955419578880 | 02:55:54.30 +08:44:58.0 (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 22.1528* 02 55 52.85 +08 44 58.6 12.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20864955419578880,2461093.6528,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 20864955419578880 20260222.1528 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:52.85 +08:44:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.11 03:04:02.95 +08:52:23.5
169.33646 -41.74828 galactic Cet Second-epoch detections are separated by 1.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 14714012495837568 | 03:04:04.02 +08:52:21.6 (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 22.1528* 03 04 02.95 +08 52 23.5 12.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 14714012495837568,2461093.6528,12.11,0.05,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 14714012495837568 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:04:02.95 +08:52:23.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.09 02:59:30.77 +01:53:09.5
174.81881 -47.66187 galactic Cet Second-epoch detections are separated by 5.9" and 9.2 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 508975100054016 | 02:59:31.18 +01:53:13.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 30.77 +01 53 09.5 12.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 508975100054016,2461093.6528,12.09,0.05,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 508975100054016 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:30.77 +01:53:09.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.24 02:57:20.36 +06:40:58.5
169.56567 -44.49261 galactic Cet Second-epoch detections are separated by 6.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8023101988151552 | 02:57:21.39 +06:40:59.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 20.36 +06 40 58.5 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8023101988151552,2461093.6528,12.24,0.05,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 8023101988151552 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:20.36 +06:40:58.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.16 02:59:45.17 +06:40:31.3
170.20541 -44.10588 galactic Cet Second-epoch detections are separated by 5.6" and 8.0 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 7284749865978368 | 02:59:45.97 +06:40:29.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 45.17 +06 40 31.3 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7284749865978368,2461093.6528,12.16,0.05,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 7284749865978368 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:45.17 +06:40:31.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.24 03:03:44.89 +01:33:56.2
176.25883 -47.13961 galactic Cet Second-epoch detections are separated by 5.8" and 8.0 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 262443977229440 | 03:03:45.36 +01:34:02.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 03 44.89 +01 33 56.2 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 262443977229440,2461093.6528,12.24,0.05,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 262443977229440 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:44.89 +01:33:56.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.13 02:55:40.66 +02:21:05.1
173.30977 -47.99090 galactic Cet Second-epoch detections are separated by 5.2" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1345596073973376 | 02:55:40.97 +02:21:13.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 40.66 +02 21 05.1 12.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1345596073973376,2461093.6528,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1345596073973376 20260222.1528 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:40.66 +02:21:05.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.16 03:00:01.93 +08:56:49.8
168.25290 -42.33330 galactic Cet Second-epoch detections are separated by 0.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8901203756936192 | 03:00:01.67 +08:56:38.2 (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 22.1528* 03 00 01.93 +08 56 49.8 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8901203756936192,2461093.6528,12.16,0.05,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 8901203756936192 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:01.93 +08:56:49.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.15 02:56:10.90 +07:26:34.0
168.57310 -44.09866 galactic Cet Second-epoch detections are separated by 1.6" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8149790639067136 | 02:56:11.84 +07:26:32.1 (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 22.1528* 02 56 10.90 +07 26 34.0 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8149790639067136,2461093.6528,12.15,0.05,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 8149790639067136 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:10.90 +07:26:34.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.25 03:00:31.18 +04:10:20.8
172.77680 -45.83588 galactic Cet Second-epoch detections are separated by 4.7" and 8.2 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 2168894060944000 | 03:00:31.86 +04:10:21.0 (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 22.1528* 03 00 31.18 +04 10 20.8 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2168894060944000,2461093.6528,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2168894060944000 20260222.1528 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:31.18 +04:10:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.16 02:55:34.96 +07:10:30.4
168.65401 -44.39924 galactic Cet Second-epoch detections are separated by 2.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8112853920328960 | 02:55:35.68 +07:10:29.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 34.96 +07 10 30.4 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8112853920328960,2461093.6528,12.16,0.05,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 8112853920328960 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:34.96 +07:10:30.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.25 02:59:29.84 +08:36:25.3
168.41120 -42.67904 galactic Cet Second-epoch detections are separated by 6.8" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8884814162243584 | 02:59:31.19 +08:36:25.1 (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 22.1528* 02 59 29.84 +08 36 25.3 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8884814162243584,2461093.6528,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8884814162243584 20260222.1528 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:29.84 +08:36:25.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.35 03:02:27.39 +09:06:15.2
168.73413 -41.82793 galactic Cet Second-epoch detections are separated by 2.4" and 8.1 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 14922988424647424 | 03:02:27.97 +09:06:19.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 02 27.39 +09 06 15.2 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 14922988424647424,2461093.6528,12.35,0.05,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 14922988424647424 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:02:27.39 +09:06:15.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.23 02:55:43.04 +07:58:50.5
167.97308 -43.75830 galactic Cet Second-epoch detections are separated by 6.2" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8372166865846912 | 02:55:44.16 +07:58:51.5 (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 22.1528* 02 55 43.04 +07 58 50.5 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8372166865846912,2461093.6528,12.23,0.05,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 8372166865846912 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:43.04 +07:58:50.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.32 03:07:12.67 +09:25:38.9
169.63891 -40.81842 galactic Cet Second-epoch detections are separated by 2.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 14851137916557056 | 03:07:13.38 +09:25:35.3 (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 22.1528* 03 07 12.67 +09 25 38.9 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 14851137916557056,2461093.6528,12.32,0.05,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
Large-amplitude variable Gaia DR2 14851137916557056 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:12.67 +09:25:38.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.22 02:59:21.95 +08:05:36.2
168.82843 -43.09308 galactic Cet Second-epoch detections are separated by 2.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8571075391208064 | 02:59:23.29 +08:05:36.4 (Gaia DR3) | ROT (local) | (local) | 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 22.1528* 02 59 21.95 +08 05 36.2 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8571075391208064,2461093.6528,12.22,0.05,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 8571075391208064 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:21.95 +08:05:36.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 59 19.19 +06 43 39.9 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LV Cet,2461093.6528,12.27,0.05,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
LV Cet 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:19.19 +06:43:39.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.34 03:00:07.89 +06:29:11.5
170.47749 -44.18579 galactic Cet Second-epoch detections are separated by 4.6" and 8.6 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 7211220025911808 | 03:00:08.46 +06:29:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 07.89 +06 29 11.5 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7211220025911808,2461093.6528,12.34,0.05,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 7211220025911808 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:07.89 +06:29:11.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.31 03:05:03.95 +10:43:52.5
167.99798 -40.16917 galactic Ari Second-epoch detections are separated by 3.6" 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 | Gaia DR3 27207179006896896 | 03:05:04.91 +10:43:48.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 05 03.95 +10 43 52.5 12.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 27207179006896896,2461093.6528,12.31,0.05,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 27207179006896896 20260222.1528 12.31CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:05:03.95 +10:43:52.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.28 02:56:10.86 +06:36:37.9
169.32474 -44.73460 galactic Cet Second-epoch detections are separated by 4.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7931533285417344 | 02:56:11.79 +06:36:43.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 10.86 +06 36 37.9 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7931533285417344,2461093.6528,12.28,0.05,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 7931533285417344 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:10.86 +06:36:37.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.26 03:03:41.88 +01:49:42.3
175.97098 -46.96422 galactic Cet Second-epoch detections are separated by 3.6" and 8.6 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 655107067371520 | 03:03:42.48 +01:49:49.2 (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 22.1528* 03 03 41.88 +01 49 42.3 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 655107067371520,2461093.6528,12.26,0.05,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 655107067371520 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:41.88 +01:49:42.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.35 03:07:14.37 +10:04:46.6
169.08415 -40.32066 galactic Cet Second-epoch detections are separated by 2.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15098287514200704 | 03:07:15.16 +10:04:42.7 (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 22.1528* 03 07 14.37 +10 04 46.6 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15098287514200704,2461093.6528,12.35,0.05,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 15098287514200704 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:14.37 +10:04:46.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.28 03:08:03.60 +10:31:03.5
168.91134 -39.85685 galactic Ari Second-epoch detections are separated by 5.1" and 8.4 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 15502568491521152 | 03:08:04.18 +10:30:56.1 (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 22.1528* 03 08 03.60 +10 31 03.5 12.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15502568491521152,2461093.6528,12.28,0.05,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 15502568491521152 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:03.60 +10:31:03.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.32 03:01:09.60 +09:34:27.2
168.00083 -41.67333 galactic Cet Second-epoch detections are separated by 7.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15008956490031872 | 03:01:10.80 +09:34:25.9 (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 22.1528* 03 01 09.60 +09 34 27.2 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15008956490031872,2461093.6528,12.32,0.05,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 15008956490031872 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:09.60 +09:34:27.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.33 03:00:38.56 +04:56:32.1
172.06287 -45.24977 galactic Cet Second-epoch detections are separated by 3.8" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 6764264253628544 | 03:00:39.07 +04:56:37.6 (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) 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 22.1528* 03 00 38.56 +04 56 32.1 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 6764264253628544,2461093.6528,12.33,0.05,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
Large-amplitude variable Gaia DR2 6764264253628544 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:38.56 +04:56:32.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.34 03:00:19.03 +06:55:50.4
170.11860 -43.82145 galactic Cet Second-epoch detections are separated by 4.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7298425041838464 | 03:00:20.14 +06:55:47.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 19.03 +06 55 50.4 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7298425041838464,2461093.6528,12.34,0.05,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 7298425041838464 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:19.03 +06:55:50.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.41 02:54:32.60 +02:37:24.8
172.72285 -47.98576 galactic Cet Second-epoch detections are separated by 5.4" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1555675809991936 | 02:54:33.43 +02:36:51.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1949TOYal..20.....B BD+02 446
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 54 32.60 +02 37 24.8 12.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1555675809991936,2461093.6528,12.41,0.05,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 1555675809991936 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:54:32.60 +02:37:24.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.44 02:59:02.74 +01:43:49.5
174.85709 -47.85465 galactic Cet Second-epoch detections are separated by 3.2" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 502962146044416 | 02:59:03.26 +01:43:56.1 (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 22.1528* 02 59 02.74 +01 43 49.5 12.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 502962146044416,2461093.6528,12.44,0.05,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 502962146044416 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:02.74 +01:43:49.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.42 02:58:59.92 +02:05:21.1
174.47168 -47.60634 galactic Cet Second-epoch detections are separated by 1.7" and 8.4 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 550653462688768 | 02:59:00.42 +02:05:21.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 59.92 +02 05 21.1 12.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 550653462688768,2461093.6528,12.42,0.05,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 550653462688768 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:59.92 +02:05:21.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.44 03:00:04.63 +08:01:20.3
169.07516 -43.03340 galactic Cet Second-epoch detections are separated by 1.8" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8557331495860736 | 03:00:05.55 +08:01:19.5 (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 22.1528* 03 00 04.63 +08 01 20.3 12.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8557331495860736,2461093.6528,12.44,0.05,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 8557331495860736 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:04.63 +08:01:20.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.46 03:04:17.92 +01:53:40.7
176.05622 -46.81087 galactic Cet Second-epoch detections are separated by 6.8" and 9.2 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 661497978703872 | 03:04:18.44 +01:53:45.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 04 17.92 +01 53 40.7 12.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 661497978703872,2461093.6528,12.46,0.05,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 661497978703872 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:04:17.92 +01:53:40.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.46 02:55:42.07 +06:33:54.6
169.23832 -44.84639 galactic Cet Second-epoch detections are separated by 5.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7936966419653376 | 02:55:42.66 +06:34:02.7 (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 22.1528* 02 55 42.07 +06 33 54.6 12.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7936966419653376,2461093.6528,12.46,0.05,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 7936966419653376 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:42.07 +06:33:54.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 07 04.56 +09 22 49.6 12.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 14849458584560256,2461093.6528,12.45,0.05,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 14849458584560256 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:04.56 +09:22:49.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.47 03:08:39.46 +10:21:21.9
169.19377 -39.88346 galactic Cet Second-epoch detections are separated by 8.3" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15484628412413312 | 03:08:40.19 +10:21:16.4 (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 22.1528* 03 08 39.46 +10 21 21.9 12.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15484628412413312,2461093.6528,12.47,0.05,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 15484628412413312 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:39.46 +10:21:21.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.46 02:56:34.92 +06:52:25.2
169.19166 -44.46970 galactic Cet Second-epoch detections are separated by 3.1" and 8.4 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 8043206730704384 | 02:56:35.40 +06:52:25.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 34.92 +06 52 25.2 12.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8043206730704384,2461093.6528,12.46,0.05,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 8043206730704384 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:34.92 +06:52:25.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.51 02:55:10.45 +06:45:30.3
168.92151 -44.78346 galactic Cet Second-epoch detections are separated by 7.4" 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 7995785996162688 | 02:55:11.10 +06:45:31.4 (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 22.1528* 02 55 10.45 +06 45 30.3 12.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7995785996162688,2461093.6528,12.51,0.05,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 7995785996162688 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:10.45 +06:45:30.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.55 02:54:59.90 +07:10:06.7
168.50416 -44.49726 galactic Cet Second-epoch detections are separated by 5.9" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8115087303325312 | 02:55:00.41 +07:10:07.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 54 59.90 +07 10 06.7 12.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8115087303325312,2461093.6528,12.55,0.05,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 8115087303325312 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:54:59.90 +07:10:06.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.52 02:57:35.03 +06:25:56.7
169.85979 -44.64272 galactic Cet Second-epoch detections are separated by 1.3" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7171912485214208 | 02:57:35.89 +06:25:50.8 (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 22.1528* 02 57 35.03 +06 25 56.7 12.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7171912485214208,2461093.6528,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 7171912485214208 20260222.1528 12.52CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:35.03 +06:25:56.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.54 02:55:53.94 +07:56:29.2
168.05570 -43.75996 galactic Cet Second-epoch detections are separated by 2.0" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8368696532272768 | 02:55:54.68 +07:56:27.3 (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 22.1528* 02 55 53.94 +07 56 29.2 12.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8368696532272768,2461093.6528,12.54,0.05,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 8368696532272768 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:53.94 +07:56:29.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.65 03:10:06.73 +10:49:44.3
169.14342 -39.29196 galactic Ari Second-epoch detections are separated by 6.5" and 8.7 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 | Large-amplitude variable Gaia DR2 15531224513293440 | 03:10:07.42 +10:49:42.1 (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 22.1528* 03 10 06.73 +10 49 44.3 12.7 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 15531224513293440,2461093.6528,12.65,0.05,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
Large-amplitude variable Gaia DR2 15531224513293440 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:10:06.73 +10:49:44.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.67 02:58:06.51 +04:15:45.8
172.05275 -46.17739 galactic Cet Second-epoch detections are separated by 7.3" and 8.5 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 2206376239593472 | 02:58:06.87 +04:15:48.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 06.51 +04 15 45.8 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2206376239593472,2461093.6528,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2206376239593472 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:06.51 +04:15:45.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.68 03:08:13.12 +10:27:57.6
168.99372 -39.87063 galactic Ari Second-epoch detections are separated by 2.1" and 8.0 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 15501091022773376 | 03:08:13.70 +10:27:49.8 (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 22.1528* 03 08 13.12 +10 27 57.6 12.7 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15501091022773376,2461093.6528,12.68,0.05,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 15501091022773376 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:13.12 +10:27:57.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.62 02:58:01.01 +04:03:51.3
172.22230 -46.33917 galactic Cet Second-epoch detections are separated by 3.4" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2199199350151040 | 02:58:01.26 +04:03:58.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 01.01 +04 03 51.3 12.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2199199350151040,2461093.6528,12.62,0.05,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 2199199350151040 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:01.01 +04:03:51.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.64 02:56:00.58 +08:20:54.8
167.72780 -43.42815 galactic Cet Second-epoch detections are separated by 2.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8809635054654464 | 02:56:01.01 +08:20:51.9 (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 22.1528* 02 56 00.58 +08 20 54.8 12.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8809635054654464,2461093.6528,12.64,0.05,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 8809635054654464 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:00.58 +08:20:54.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.71 02:57:25.76 +09:21:31.7
167.22727 -42.42353 galactic Cet Second-epoch detections are separated by 7.1" and 8.8 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 20996965534503680 | 02:57:26.29 +09:21:27.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K2 (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 22.1528* 02 57 25.76 +09 21 31.7 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20996965534503680,2461093.6528,12.71,0.05,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 20996965534503680 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:25.76 +09:21:31.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.59 03:04:18.42 +10:06:38.1
168.33420 -40.76466 galactic Cet Second-epoch detections are separated by 4.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15136705997268224 | 03:04:19.32 +10:06:33.8 (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 22.1528* 03 04 18.42 +10 06 38.1 12.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15136705997268224,2461093.6528,12.59,0.05,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 15136705997268224 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:04:18.42 +10:06:38.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.70 02:56:46.07 +06:35:13.1
169.50213 -44.65783 galactic Cet Second-epoch detections are separated by 2.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7928818866087168 | 02:56:46.44 +06:35:15.1 (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 22.1528* 02 56 46.07 +06 35 13.1 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7928818866087168,2461093.6528,12.70,0.05,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 7928818866087168 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:46.07 +06:35:13.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.64 02:57:29.05 +09:10:22.3
167.40056 -42.55929 galactic Cet Second-epoch detections are separated by 0.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 20974047588869632 | 02:57:29.53 +09:10:19.4 (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 22.1528* 02 57 29.05 +09 10 22.3 12.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20974047588869632,2461093.6528,12.64,0.05,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 20974047588869632 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:29.05 +09:10:22.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.71 03:03:33.42 +10:28:16.0
167.84261 -40.60636 galactic Ari Second-epoch detections are separated by 3.4" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 27172986771940992 | 03:03:33.99 +10:28:12.6 (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 22.1528* 03 03 33.42 +10 28 16.0 12.7 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 27172986771940992,2461093.6528,12.71,0.05,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 27172986771940992 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:03:33.42 +10:28:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.71 02:57:41.71 +09:19:29.7
167.32516 -42.40849 galactic Cet Second-epoch detections are separated by 6.1" and 8.4 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 20984149351945856 | 02:57:42.57 +09:19:24.9 (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 22.1528* 02 57 41.71 +09 19 29.7 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20984149351945856,2461093.6528,12.71,0.05,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 20984149351945856 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:41.71 +09:19:29.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.59 02:57:11.55 +05:55:21.5
170.22796 -45.09132 galactic Cet Second-epoch detections are separated by 8.1" and 9.3 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 7071547689461888 | 02:57:12.26 +05:55:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 11.55 +05 55 21.5 12.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7071547689461888,2461093.6528,12.59,0.05,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 7071547689461888 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:11.55 +05:55:21.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.69 02:56:40.72 +06:31:51.8
169.52966 -44.71470 galactic Cet Second-epoch detections are separated by 2.6" and 8.4 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 7926349260516480 | 02:56:41.39 +06:31:55.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 40.72 +06 31 51.8 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7926349260516480,2461093.6528,12.69,0.05,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 7926349260516480 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:40.72 +06:31:51.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.78 03:01:56.46 +09:21:13.9
168.38797 -41.71905 galactic Cet Second-epoch detections are separated by 6.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 14943569907922048 | 03:01:56.87 +09:21:12.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 56.46 +09 21 13.9 12.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 14943569907922048,2461093.6528,12.78,0.05,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 14943569907922048 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:56.46 +09:21:13.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.71 02:55:51.25 +09:28:24.6
166.71929 -42.57783 galactic Cet Second-epoch detections are separated by 2.4" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 21046993313391872 | 02:55:51.78 +09:28:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 51.25 +09 28 24.6 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 21046993313391872,2461093.6528,12.71,0.05,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 21046993313391872 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:51.25 +09:28:24.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.71 02:59:32.12 +08:46:25.1
168.27583 -42.54516 galactic Cet Second-epoch detections are separated by 3.1" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8891441296574720 | 02:59:32.63 +08:46:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 32.12 +08 46 25.1 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8891441296574720,2461093.6528,12.71,0.05,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 8891441296574720 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:32.12 +08:46:25.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.79 02:56:43.82 +07:32:34.6
168.62864 -43.93455 galactic Cet Second-epoch detections are separated by 6.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8152470698686336 | 02:56:44.40 +07:32:28.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 43.82 +07 32 34.6 12.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8152470698686336,2461093.6528,12.79,0.05,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 8152470698686336 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:43.82 +07:32:34.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.79 02:54:51.53 +03:14:11.0
172.19128 -47.48183 galactic Cet Second-epoch detections are separated by 6.2" and 8.4 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 1667031426894464 | 02:54:51.68 +03:14:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 22.1528* 02 54 51.53 +03 14 11.0 12.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1667031426894464,2461093.6528,12.79,0.05,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 1667031426894464 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:54:51.53 +03:14:11.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.72 02:57:42.56 +05:07:42.3
171.11296 -45.60168 galactic Cet Second-epoch detections are separated by 3.7" and 8.1 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 5329337155355008 | 02:57:43.22 +05:07:46.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 42.56 +05 07 42.3 12.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5329337155355008,2461093.6528,12.72,0.05,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 5329337155355008 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:42.56 +05:07:42.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 56 39.12 +07 45 02.0 12.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8350795108587904,2461093.6528,12.83,0.05,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 8350795108587904 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:39.12 +07:45:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.93 03:00:08.88 +09:09:17.4
168.10305 -42.15543 galactic Cet Second-epoch detections are separated by 2.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8975725734788736 | 03:00:09.56 +09:09:13.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 08.88 +09 09 17.4 12.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8975725734788736,2461093.6528,12.93,0.05,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 8975725734788736 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:08.88 +09:09:17.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.89 02:58:50.41 +11:04:11.0
166.15757 -40.87146 galactic Ari Second-epoch detections are separated by 7.4" and 9.3 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 27466148354792320 | 02:58:50.05 +11:04:07.5 (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 22.1528* 02 58 50.41 +11 04 11.0 12.9 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 27466148354792320,2461093.6528,12.89,0.05,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 27466148354792320 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:50.41 +11:04:11.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.87 02:59:50.18 +08:39:15.4
168.45727 -42.58902 galactic Cet Second-epoch detections are separated by 1.2" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8875051701374976 | 02:59:50.99 +08:39:08.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 50.18 +08 39 15.4 12.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8875051701374976,2461093.6528,12.87,0.05,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 8875051701374976 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:50.18 +08:39:15.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.86 02:58:43.18 +07:30:54.9
169.17505 -43.63747 galactic Cet Second-epoch detections are separated by 2.5" and 8.0 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 8514789844194816 | 02:58:44.35 +07:30:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 43.18 +07 30 54.9 12.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8514789844194816,2461093.6528,12.86,0.05,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 8514789844194816 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:43.18 +07:30:54.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.93 02:57:21.53 +08:31:15.9
167.93124 -43.08300 galactic Cet Second-epoch detections are separated by 4.0" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8834683303945088 | 02:57:22.26 +08:31:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 21.53 +08 31 15.9 12.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8834683303945088,2461093.6528,12.93,0.05,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 8834683303945088 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:21.53 +08:31:15.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.87 02:57:28.61 +09:30:30.4
167.11213 -42.29987 galactic Cet Second-epoch detections are separated by 2.4" and 8.1 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 21003562604119168 | 02:57:28.21 +09:30:31.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 22.1528* 02 57 28.61 +09 30 30.4 12.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 21003562604119168,2461093.6528,12.87,0.05,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 21003562604119168 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:28.61 +09:30:30.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 55 12.60 +07 58 16.3 13.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J025513.02+075811.9,2461093.6528,12.97,0.05,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
ASASSN-V J025513.02+075811.9 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:12.60 +07:58:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.12 02:56:21.38 +05:03:29.6
170.81897 -45.87798 galactic Cet Second-epoch detections are separated by 2.5" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5335414533530496 | 02:56:20.96 +05:03:28.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 21.38 +05 03 29.6 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5335414533530496,2461093.6528,13.12,0.05,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 5335414533530496 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:21.38 +05:03:29.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.00 02:56:55.98 +07:27:40.5
168.75505 -43.96480 galactic Cet Second-epoch detections are separated by 0.8" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8148003932700288 | 02:56:56.37 +07:27:36.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 55.98 +07 27 40.5 13.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8148003932700288,2461093.6528,13.00,0.05,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 8148003932700288 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:55.98 +07:27:40.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.07 02:57:31.75 +09:43:00.6
166.94894 -42.12963 galactic Cet Second-epoch detections are separated by 4.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 21078054516894976 | 02:57:31.14 +09:43:01.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 31.75 +09 43 00.6 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 21078054516894976,2461093.6528,13.07,0.05,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 21078054516894976 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:31.75 +09:43:00.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.01 02:58:45.92 +05:34:00.3
170.97707 -45.09958 galactic Cet Second-epoch detections are separated by 4.6" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 6855970395322112 | 02:58:46.46 +05:33:51.9 (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 22.1528* 02 58 45.92 +05 34 00.3 13.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 6855970395322112,2461093.6528,13.01,0.05,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 6855970395322112 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:45.92 +05:34:00.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 54 42.71 +03 48 09.1 13.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.46,0.05,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
VARIABLE_NAME 20260222.1528 13.46CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:42.71 +03:48:09.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.16 02:59:49.76 +08:39:22.7
168.45370 -42.58857 galactic Cet Second-epoch detections are separated by 4.0" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8875051701374976 | 02:59:50.99 +08:39:08.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 49.76 +08 39 22.7 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8875051701374976,2461093.6528,13.16,0.05,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 8875051701374976 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:49.76 +08:39:22.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.95 02:56:45.63 +08:58:09.7
167.38683 -42.82990 galactic Cet Second-epoch detections are separated by 2.3" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 20875808801489920 | 02:56:47.17 +08:58:12.0 (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 22.1528* 02 56 45.63 +08 58 09.7 12.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20875808801489920,2461093.6528,12.95,0.05,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 20875808801489920 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:45.63 +08:58:09.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.03 02:58:43.82 +07:30:56.8
169.17736 -43.63535 galactic Cet Second-epoch detections are separated by 0.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8514789844194816 | 02:58:44.35 +07:30:52.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 43.82 +07 30 56.8 13.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8514789844194816,2461093.6528,13.03,0.05,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 8514789844194816 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:43.82 +07:30:56.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.87 02:56:23.14 +10:02:52.0
166.37405 -42.04702 galactic Cet Second-epoch detections are separated by 6.4" and 8.8 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 21289504346955264 | 02:56:22.59 +10:02:55.1 (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 22.1528* 02 56 23.14 +10 02 52.0 12.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 21289504346955264,2461093.6528,12.87,0.05,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 21289504346955264 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:23.14 +10:02:52.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.16 02:55:57.36 +05:48:24.1
170.00653 -45.38062 galactic Cet Second-epoch detections are separated by 4.3" and 8.1 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 7110541696842240 | 02:55:57.41 +05:48:17.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 57.36 +05 48 24.1 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7110541696842240,2461093.6528,13.16,0.05,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 7110541696842240 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:57.36 +05:48:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.09 02:57:21.79 +08:31:16.9
167.93213 -43.08210 galactic Cet Second-epoch detections are separated by 5.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8834683303945088 | 02:57:22.26 +08:31:14.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 21.79 +08 31 16.9 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8834683303945088,2461093.6528,13.09,0.05,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 8834683303945088 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:21.79 +08:31:16.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.10 03:01:37.89 +01:39:16.5
175.61718 -47.45321 galactic Cet Second-epoch detections are separated by 6.7" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 461142048768128 | 03:01:38.59 +01:39:22.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G8 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 01 37.89 +01 39 16.5 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 461142048768128,2461093.6528,13.10,0.05,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 461142048768128 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:37.89 +01:39:16.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.04 03:06:37.50 +08:33:57.7
170.24881 -41.56165 galactic Cet Second-epoch detections are separated by 4.1" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 13895146916018048 | 03:06:37.59 +08:33:43.4 (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 22.1528* 03 06 37.50 +08 33 57.7 13.0 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 13895146916018048,2461093.6528,13.04,0.05,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 13895146916018048 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:06:37.50 +08:33:57.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.07 02:56:29.06 +08:15:07.9
167.93696 -43.42805 galactic Cet Second-epoch detections are separated by 5.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8804923474975616 | 02:56:29.49 +08:15:07.8 (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 22.1528* 02 56 29.06 +08 15 07.9 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8804923474975616,2461093.6528,13.07,0.05,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 8804923474975616 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:29.06 +08:15:07.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.08 03:00:26.32 +09:32:43.1
167.84205 -41.80907 galactic Cet Second-epoch detections are separated by 2.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 15010674476916736 | 03:00:27.06 +09:32:38.0 (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 22.1528* 03 00 26.32 +09 32 43.1 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 15010674476916736,2461093.6528,13.08,0.05,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 15010674476916736 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:26.32 +09:32:43.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.10 02:55:32.55 +05:39:00.1
170.04208 -45.56637 galactic Cet Second-epoch detections are separated by 7.2" and 9.1 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 5605555092189952 | 02:55:32.14 +05:38:55.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 32.55 +05 39 00.1 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5605555092189952,2461093.6528,13.10,0.05,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 5605555092189952 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:32.55 +05:39:00.1 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.09 02:55:00.02 +05:08:34.7
170.37377 -46.03737 galactic Cet Second-epoch detections are separated by 2.4" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5505392159247104 | 02:54:59.63 +05:08:29.6 (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 22.1528* 02 55 00.02 +05 08 34.7 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5505392159247104,2461093.6528,13.09,0.05,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 5505392159247104 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:00.02 +05:08:34.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.24 02:58:33.50 +06:32:57.8
170.00881 -44.39576 galactic Cet Second-epoch detections are separated by 4.4" and 8.5 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 7256639304498176 | 02:58:34.03 +06:32:57.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 33.50 +06 32 57.8 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7256639304498176,2461093.6528,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 7256639304498176 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:33.50 +06:32:57.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.19 02:59:54.00 +09:33:22.5
167.69518 -41.88513 galactic Cet Second-epoch detections are separated by 2.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 9006924376892544 | 02:59:54.45 +09:33:17.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 54.00 +09 33 22.5 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 9006924376892544,2461093.6528,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 9006924376892544 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:54.00 +09:33:22.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.18 02:57:00.98 +10:18:57.8
166.31342 -41.74039 galactic Cet Second-epoch detections are separated by 3.2" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 27308020547044864 | 02:57:00.56 +10:19:02.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE 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 22.1528* 02 57 00.98 +10 18 57.8 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 27308020547044864,2461093.6528,13.18,0.05,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 27308020547044864 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:00.98 +10:18:57.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.09 02:56:46.27 +08:58:16.0
167.38811 -42.82688 galactic Cet Second-epoch detections are separated by 2.8" and 8.1 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 20875808801489920 | 02:56:47.17 +08:58:12.0 (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 22.1528* 02 56 46.27 +08 58 16.0 13.1 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20875808801489920,2461093.6528,13.09,0.05,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 20875808801489920 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:46.27 +08:58:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.20 02:56:16.75 +02:23:25.3
173.43285 -47.85941 galactic Cet Second-epoch detections are separated by 5.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1351162351587072 | 02:56:17.04 +02:23:35.9 (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 22.1528* 02 56 16.75 +02 23 25.3 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1351162351587072,2461093.6528,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1351162351587072 20260222.1528 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:16.75 +02:23:25.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.23 02:57:44.59 +04:12:40.7
172.00568 -46.27679 galactic Cet Second-epoch detections are separated by 8.3" and 8.4 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 2204486453985024 | 02:57:45.01 +04:12:37.5 (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 22.1528* 02 57 44.59 +04 12 40.7 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2204486453985024,2461093.6528,13.23,0.05,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 2204486453985024 20260222.1528 13.23CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:44.59 +04:12:40.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.18 02:57:09.71 +09:07:06.7
167.36333 -42.65165 galactic Cet Second-epoch detections are separated by 2.8" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 20971947349799552 | 02:57:10.35 +09:07:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 09.71 +09 07 06.7 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20971947349799552,2461093.6528,13.18,0.05,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 20971947349799552 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:09.71 +09:07:06.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.35 02:56:28.13 +07:58:26.8
168.17726 -43.64485 galactic Cet Second-epoch detections are separated by 6.6" and 8.5 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 8743728781351808 | 02:56:28.55 +07:58:24.3 (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 22.1528* 02 56 28.13 +07 58 26.8 13.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8743728781351808,2461093.6528,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8743728781351808 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:28.13 +07:58:26.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.32 02:57:52.14 +08:54:55.3
167.72209 -42.69846 galactic Cet Second-epoch detections are separated by 8.3" and 9.1 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 8955694007171968 | 02:57:52.89 +08:54:48.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 52.14 +08 54 55.3 13.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8955694007171968,2461093.6528,13.32,0.05,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 8955694007171968 20260222.1528 13.32CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:52.14 +08:54:55.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.37 02:56:32.99 +03:38:58.6
172.23807 -46.89207 galactic Cet 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 2056911377677056 | 02:56:33.55 +03:39:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 32.99 +03 38 58.6 13.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2056911377677056,2461093.6528,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2056911377677056 20260222.1528 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:32.99 +03:38:58.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.21 02:59:21.49 +08:29:43.5
168.47284 -42.78670 galactic Cet Second-epoch detections are separated by 7.4" 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 8778161534503680 | 02:59:21.97 +08:29:41.6 (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 22.1528* 02 59 21.49 +08 29 43.5 13.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8778161534503680,2461093.6528,13.21,0.05,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 8778161534503680 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:21.49 +08:29:43.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 55 12.29 +03 58 25.6 13.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5082973536079872,2461093.6528,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5082973536079872 20260222.1528 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:12.29 +03:58:25.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.51 02:54:58.43 +06:39:42.5
168.95572 -44.88938 galactic Cet Second-epoch detections are separated by 5.0" and 7.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 7942013005618176 | 02:54:58.91 +06:39:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G9 (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 22.1528* 02 54 58.43 +06 39 42.5 13.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7942013005618176,2461093.6528,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 7942013005618176 20260222.1528 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:54:58.43 +06:39:42.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.35 02:56:17.09 +08:50:58.7
167.36547 -42.99690 galactic Cet Second-epoch detections are separated by 3.5" and 8.2 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 20867493744806528 | 02:56:17.87 +08:50:59.1 (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 22.1528* 02 56 17.09 +08 50 58.7 13.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 20867493744806528,2461093.6528,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 20867493744806528 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:17.09 +08:50:58.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 56 12.42 +03 11 47.8 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:12.42 +03:11:47.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.48 02:56:38.19 +04:11:58.9
171.72113 -46.47102 galactic Cet Second-epoch detections are separated by 7.9" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5114309617465600 | 02:56:38.15 +04:12:04.9 (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 22.1528* 02 56 38.19 +04 11 58.9 13.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5114309617465600,2461093.6528,13.48,0.05,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
Gaia DR3 5114309617465600 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:38.19 +04:11:58.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.35 02:59:10.30 +10:42:38.3
166.53822 -41.10168 galactic Ari Second-epoch detections are separated by 2.5" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 27348191373038336 | 02:59:10.63 +10:42:31.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 10.30 +10 42 38.3 13.3 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 27348191373038336,2461093.6528,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 27348191373038336 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:10.30 +10:42:38.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.39 02:55:34.42 +03:04:54.8
172.54034 -47.47470 galactic Cet Second-epoch detections are separated by 5.5" and 8.0 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 1611265571527936 | 02:55:34.57 +03:05:00.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 34.42 +03 04 54.8 13.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1611265571527936,2461093.6528,13.39,0.05,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 1611265571527936 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:34.42 +03:04:54.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.46 02:55:47.39 +04:23:25.6
171.30806 -46.47056 galactic Cet Second-epoch detections are separated by 7.4" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 5135234698128640 | 02:55:47.27 +04:23:32.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 47.39 +04 23 25.6 13.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5135234698128640,2461093.6528,13.46,0.05,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 5135234698128640 20260222.1528 13.46CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:47.39 +04:23:25.6 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.44 03:00:13.07 +02:29:49.2
174.37448 -47.10164 galactic Cet Second-epoch detections are separated by 4.1" and 8.6 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 | 03:00:13.07 +02:29:49.2 (user input) | T | P | (position from user input) SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 13.07 +02 29 49.2 13.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:13.07 +02:29:49.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.72 03:00:08.75 +02:26:30.9
174.41193 -47.15368 galactic Cet Second-epoch detections are separated by 6.9" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:00:08.75 +02:26:30.9 (user input) | T | P | (position from user input) SpType: F6 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 08.75 +02 26 30.9 13.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:08.75 +02:26:30.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 00 49.95 +02 07 34.3 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:49.95 +02:07:34.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.45 02:55:46.62 +09:23:51.4
166.76350 -42.64899 galactic Cet Second-epoch detections are separated by 4.6" and 8.2 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 21042006855788928 | 02:55:47.28 +09:23:47.1 (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 22.1528* 02 55 46.62 +09 23 51.4 13.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 21042006855788928,2461093.6528,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 21042006855788928 20260222.1528 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:46.62 +09:23:51.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.55 02:56:19.18 +05:05:07.9
170.78317 -45.86358 galactic Cet Second-epoch detections are separated by 3.2" and 8.2 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 5335792490652416 | 02:56:18.80 +05:05:09.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 19.18 +05 05 07.9 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 5335792490652416,2461093.6528,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 5335792490652416 20260222.1528 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:19.18 +05:05:07.9 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.49 02:59:14.85 +09:24:35.1
167.65317 -42.10048 galactic Cet Second-epoch detections are separated by 2.4" and 8.0 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 8998162643550336 | 02:59:15.24 +09:24:29.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 59 14.85 +09 24 35.1 13.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8998162643550336,2461093.6528,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8998162643550336 20260222.1528 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:14.85 +09:24:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.57 02:56:33.61 +03:38:56.3
172.24148 -46.89080 galactic Cet Second-epoch detections are separated by 4.1" and 8.1 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 2056911377677056 | 02:56:33.55 +03:39:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 33.61 +03 38 56.3 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2056911377677056,2461093.6528,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2056911377677056 20260222.1528 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:33.61 +03:38:56.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.60 03:00:29.52 +04:51:26.8
172.10500 -45.33764 galactic Cet Second-epoch detections are separated by 3.3" and 8.5 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 | 03:00:29.52 +04:51:26.8 (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 22.1528* 03 00 29.52 +04 51 26.8 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.60,0.05,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 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:29.52 +04:51:26.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.53 02:56:54.35 +09:32:25.2
166.93683 -42.36346 galactic Cet Second-epoch detections are separated by 2.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J044.2293+09.5382 | 02:56:55.04 +09:32:17.5 (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 22.1528* 02 56 54.35 +09 32 25.2 13.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J044.2293+09.5382,2461093.6528,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J044.2293+09.5382 20260222.1528 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:54.35 +09:32:25.2 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.47 02:55:13.22 +04:01:40.8
171.50692 -46.83511 galactic Cet Second-epoch detections are separated by 4.0" and 8.1 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 J043.8078+04.0278 | 02:55:13.87 +04:01:40.1 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 55 13.22 +04 01 40.8 13.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J043.8078+04.0278,2461093.6528,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J043.8078+04.0278 20260222.1528 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:13.22 +04:01:40.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.63 02:56:00.70 +02:31:46.5
173.21813 -47.80401 galactic Cet Second-epoch detections are separated by 8.7" 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 1366903407519104 | 02:56:00.82 +02:31:53.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G2 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 00.70 +02 31 46.5 13.6 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1366903407519104,2461093.6528,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1366903407519104 20260222.1528 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:00.70 +02:31:46.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.51 03:00:57.43 +09:20:44.8
168.14519 -41.88094 galactic Cet Second-epoch detections are separated by 1.9" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 8985041519036032 | 03:00:58.14 +09:20:44.1 (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 22.1528* 03 00 57.43 +09 20 44.8 13.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 8985041519036032,2461093.6528,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 8985041519036032 20260222.1528 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:57.43 +09:20:44.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.66 02:57:24.89 +02:11:05.3
173.95006 -47.81252 galactic Cet Second-epoch detections are separated by 8.0" and 9.5 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 1294022106687744 | 02:57:25.53 +02:11:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F9 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 57 24.89 +02 11 05.3 13.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1294022106687744,2461093.6528,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1294022106687744 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:24.89 +02:11:05.3 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 54 36.69 +03 25 36.5 13.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:54:36.69 +03:25:36.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.69 02:56:12.32 +09:28:07.5
166.81509 -42.52743 galactic Cet Second-epoch detections are separated by 1.1" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 21044240238780800 | 02:56:12.81 +09:28:03.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 12.32 +09 28 07.5 13.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 21044240238780800,2461093.6528,13.69,0.05,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 21044240238780800 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:12.32 +09:28:07.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 58 08.35 +08 29 43.4 13.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:08.35 +08:29:43.4 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.70 02:56:51.75 +07:49:26.7
168.41350 -43.69788 galactic Cet Second-epoch detections are separated by 7.0" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J044.2193+07.8263 | 02:56:52.20 +07:49:26.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 56 51.75 +07 49 26.7 13.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J044.2193+07.8263,2461093.6528,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J044.2193+07.8263 20260222.1528 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:56:51.75 +07:49:26.7 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.74 02:58:31.58 +07:00:19.1
169.58431 -44.05607 galactic Cet Second-epoch detections are separated by 4.0" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 02:58:31.58 +07:00:19.1 (user input) | T | P | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 58 31.58 +07 00 19.1 13.7 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:58:31.58 +07:00:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 13.80 02:55:57.49 +01:47:16.8
173.96818 -48.35082 galactic Cet Second-epoch detections are separated by 6.3" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1175584089096960 | 02:55:58.21 +01:47:20.7 (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 22.1528* 02 55 57.49 +01 47 16.8 13.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1175584089096960,2461093.6528,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1175584089096960 20260222.1528 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:55:57.49 +01:47:16.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 02 59 14.88 +05 43 36.0 13.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461093.6528,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.1528 13.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:14.88 +05:43:36.0 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 32 32.81 +07 25 31.8 9.8 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J033233+0725.5,2461093.6528,9.85,0.05,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
ASAS J033233+0725.5 20260222.1528 9.85CV 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:32.81 +07:25:31.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 49 27.30 +06 04 41.1 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1191 Tau,2461093.6528,11.55,0.05,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
V1191 Tau 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:27.30 +06:04:41.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.26 02:54:56.68 +01:38:57.8
173.83686 -48.62610 galactic Cet Second-epoch detections are separated by 7.0" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J043.7261+01.6485 | 02:54:56.88 +01:38:58.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 02 54 56.68 +01 38 57.8 12.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J043.7261+01.6485,2461093.6528,12.26,0.05,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
ATO J043.7261+01.6485 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:54:56.68 +01:38:57.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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 22.1528* 03 43 28.67 +07 10 58.8 13.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J0343288+071058,2461093.6528,13.38,0.05,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
NSVS J0343288+071058 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:28.67 +07:10:58.8 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.1528 2461093.6528 12.75 03:00:06.39 +06:38:44.5
170.32460 -44.07033 galactic Cet Second-epoch detections are separated by 1.2" and 8.0 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 7283993951733376 | 03:00:06.84 +06:38:44.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.1528* 03 00 06.39 +06 38 44.5 12.8 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 7283993951733376,2461093.6528,12.75,0.05,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 7283993951733376 20260222.1528 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:06.39 +06:38:44.5 ;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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20_00sec_-14_90C_LIGHT_0085_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20_00sec_-15_00C_LIGHT_0244_fits__*pix.png resample_wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20_00sec_-14_90C_LIGHT_0084_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: 2461032.73017573 23.12.2025 05:31:17.183 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
First image: 2461032.73017573 23.12.2025 05:31:17.183 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
Last image: 2461093.65306700 22.02.2026 03:40:14.989 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 164
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: 3 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): 6981
Objects passed selection criteria: 6962
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 5820.75
Average stars matched: 5643 (96.9463 %)
Memory usage VmPeak: 115360 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 03:11:53 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: 2461032.73017573 23.12.2025 05:31:17.183 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
First image: 2461032.73017573 23.12.2025 05:31:17.183 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
Last image: 2461093.65306700 22.02.2026 03:40:14.989 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 771
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 25 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): 37924
Objects passed selection criteria: 37837
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 30105.2
Average stars matched: 28315.8 (94.0559 %)
Memory usage VmPeak: 139800 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 03:14:56 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:
Tau-07-Q2b1x1
#######################################
########### Starting Tau-07-Q2b1x1 ###########
Processing Tau-07-Q2b1x1
server tau has sufficient free disk space available: 1047403 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 1047403 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.png' -> 'transient_report/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits_preview.png'
Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
renamed 'Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.png' -> 'transient_report/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits_preview.png'
Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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= 622.3229
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 558.3709
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1453.4333
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 563.1550
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1455.3479
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 562.8931
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.3355
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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
SExtractor catalog cache: saved Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat to cache
SExtractor catalog cache: saved Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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: 2461093.65248898
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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits exists and is non-empty
Saving wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits to local_wcs_cache/
'wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits' -> 'local_wcs_cache/wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits'
wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits exists and is non-empty
Saving wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits to local_wcs_cache/
'wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits' -> 'local_wcs_cache/wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits'
wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits exists and is non-empty
Saving wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits to local_wcs_cache/
'wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits' -> 'local_wcs_cache/wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits'
wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits exists and is non-empty
Saving wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits to local_wcs_cache/
'wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits' -> 'local_wcs_cache/wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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 03:25:27.563 +05:58:50.42
Second-epoch image center 03:25:34.852 +06:00:24.35
Angular distance between the image centers 0.04 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 03:25:27.563 +05:58:50.42
Second-epoch image center 03:25:32.016 +06:00:04.69
Angular distance between the image centers 0.03 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 03:25:34.852 +06:00:24.35
Second-epoch second image center 03:25:32.016 +06:00:04.69
Angular distance between the image centers 0.01296 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits &> /tmp/tmp.R5kKP9URdA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits &> /tmp/tmp.yTPwjfmeWE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits &> /tmp/tmp.0n2wA9b1bA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits &> /tmp/tmp.aEbEjF65Aw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits and wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits and wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat
Found non-empty wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits and wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat
The reference image (wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits) and catalog (wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat) found
'wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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 3726 out of 7086 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.941556
a=0.000000 b=1.000000 c=22.941556
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 137 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
2.0 pix Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
3.6 pix Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
3.6 pix Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
Limiting magnitude estimates:
15.3 mag. Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
15.3 mag. Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
14.5 mag. Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
14.4 mag. Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.9 (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.R5kKP9URdA (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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits' -> 'wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
WCS_IMAGE_NAME=wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
WCS-calibrated image found: wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
Checking if the catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits alredy exist and is non-empty...
Catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
WCS catalog name: wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=502, passed=7086
Got 7086 stars (including 6577 good ones) from the SExtractor catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat
util/solve_plate_with_UCAC5 got 7086 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 970 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits -region wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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.yTPwjfmeWE (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/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits' -> 'wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
WCS_IMAGE_NAME=wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
WCS-calibrated image found: wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
Checking if the catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits alredy exist and is non-empty...
Catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
WCS catalog name: wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=500, passed=7036
Got 7036 stars (including 6528 good ones) from the SExtractor catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat
util/solve_plate_with_UCAC5 got 7036 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 970 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits -region wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.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.0n2wA9b1bA (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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
WCS_IMAGE_NAME=wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
WCS-calibrated image found: wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
Checking if the catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits alredy exist and is non-empty...
Catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
WCS catalog name: wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=560, passed=4665
Got 4665 stars (including 4104 good ones) from the SExtractor catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat
util/solve_plate_with_UCAC5 got 4665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 972 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.71"
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits -region wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.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.aEbEjF65Aw (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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
WCS_IMAGE_NAME=wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
WCS-calibrated image found: wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
Checking if the catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits alredy exist and is non-empty...
Catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
WCS catalog name: wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=571, passed=4638
Got 4638 stars (including 4062 good ones) from the SExtractor catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat
util/solve_plate_with_UCAC5 got 4638 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 970 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: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.72"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits -region wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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 Tau-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20508.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20513.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20525.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20540.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20577.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out20358.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out01133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out03071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20476.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20542.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 50s
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: 27s
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Considering the candidate 20358_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20358_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:15.70 +02:39:39.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)
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Considering the candidate 20359_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20359_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:21.63 +03:16:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 1.035 1815568575811456 044.84037262076 +03.27576994550 10.3570 9.7216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20360_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20360_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:22.40 +03:31:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 0.773 1911024224195328 045.59346661345 +03.52710906845 10.6352 10.1245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20361_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20361_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:02.01 +08:49:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 0.610 14666179444575744 046.50844298439 +08.83187211415 10.6555 10.1301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20362_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20362_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:26.19 +08:25:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 2.033 8668102996791424 045.60903683539 +08.41699748216 10.3746 9.7948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20363_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20363_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20364_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20364_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:34.72 +07:25:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 2.713 7715861503232384 045.89539658567 +07.42581744453 10.5523 10.0777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20366_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20366_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20368_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20368_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:38.88 +10:39:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 0.690 15194494781621632 046.41218248733 +10.65696035172 10.2462 9.7884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20369_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20369_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20370_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20370_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:31.84 +03:52:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.41, MAG_FAINT_SEARCH_LIMIT=12.39)GAIADR2_OUTPUT=# 1.294 1955756307917312 045.63232563880 +03.87135607712 10.1987 9.8459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20371_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20371_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:00.87 +07:18:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 1.152 8086259482884864 044.75349405725 +07.31501312455 10.0991 9.6155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20372_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20372_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:51.41 +07:44:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 0.906 8492769547504256 045.46440230116 +07.74186520782 10.3021 9.8697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20373_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20373_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:44.86 +02:33:15.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)
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Considering the candidate 20374_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20374_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:07:25.29 +10:40:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 1.919 15555379408746112 046.85578116183 +10.67856334571 10.2271 9.7784 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 20376_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20376_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20377_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20377_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:51.92 +08:23:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 2.972 8634159870901120 046.21553243345 +08.39418505029 10.2714 9.8223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20378_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20378_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20379_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20379_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20380_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20380_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20381_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20381_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20382_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20382_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20384_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20384_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:46.71 +07:16:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.23, MAG_FAINT_SEARCH_LIMIT=12.21)GAIADR2_OUTPUT=# 2.595 7698819073017600 045.44399630381 +07.27788829839 9.9767 9.5937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20386_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20386_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:09:22.51 +10:48:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.27, MAG_FAINT_SEARCH_LIMIT=12.25)GAIADR2_OUTPUT=# 5.328 15537409266205824 047.34494069904 +10.80993142325 10.0211 9.5282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20388_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20388_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20389_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20389_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20390_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20390_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20391_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20391_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:11.50 +09:06:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 5.038 14698065281775616 046.54656723753 +09.10139989560 10.0114 9.5687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20392_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20392_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20393_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20393_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:06.94 +02:07:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.93, MAG_FAINT_SEARCH_LIMIT=11.91)GAIADR2_OUTPUT=# 2.490 879991554932352 046.02832174323 +02.13261863854 9.6681 9.2574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20394_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20394_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20395_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20395_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20396_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20396_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:28.57 +05:12:36.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.89, MAG_FAINT_SEARCH_LIMIT=11.87)
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Considering the candidate 20397_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20397_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20399_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20399_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20400_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20400_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20401_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20401_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20402_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20402_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 20403_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20403_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20405_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20405_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20408_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20408_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20409_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20409_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:22.02 +06:14:51.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20410_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20410_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:13:03.48 +10:53:12.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20413_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20413_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:51.45 +06:08:00.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20414_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20414_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:42.71 +08:54:30.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20415_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20415_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:44.21 +10:52:15.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20417_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20417_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:13.03 +08:22:54.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20418_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20418_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:30.85 +02:00:59.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20419_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20419_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:07.70 +03:29:10.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20421_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20421_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:24.54 +10:47:50.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20426_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20426_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:13.59 +04:02:52.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20427_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20427_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:04.79 +10:39:24.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20429_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20429_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:14.72 +01:53:06.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20432_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20432_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:17.02 +10:12:38.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20433_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20433_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:00.30 +10:09:40.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20434_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20434_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:43.81 +11:00:51.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20435_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20435_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:36.41 +05:59:02.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20438_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20438_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:50.43 +10:30:09.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20441_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20441_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:48.14 +10:51:00.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.71, MAG_FAINT_SEARCH_LIMIT=10.69)
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Considering the candidate 20445_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20445_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:20.89 +03:19:05.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20446_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20446_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:29.84 +10:07:31.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20447_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20447_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:19.38 +11:08:13.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20448_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20448_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:46.23 +03:29:53.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20449_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20449_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:20.72 +05:28:39.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20450_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20450_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:04.77 +07:39:11.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20451_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20451_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:50.23 +07:31:35.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20453_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20453_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:21.40 +10:28:51.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20455_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20455_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:56.90 +10:38:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.16, MAG_FAINT_SEARCH_LIMIT=11.14)GAIADR2_OUTPUT=# 0.551 27334687995840000 044.23696568813 +10.64526716186 8.5665 7.7853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.551#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20456_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20456_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:28.58 +07:46:40.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20457_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20457_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:46.49 +03:34:05.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20459_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20459_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20460_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20460_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:16.77 +05:59:49.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20461_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20461_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20464_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20464_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20465_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20465_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20466_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20466_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20467_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20467_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20468_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20468_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:09.19 +10:32:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.55, MAG_FAINT_SEARCH_LIMIT=11.53)GAIADR2_OUTPUT=# 1.327 27329770258039296 044.28801227425 +10.54144020455 9.0116 8.2093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20471_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20471_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20472_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20472_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:55.25 +05:35:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.65, MAG_FAINT_SEARCH_LIMIT=11.63)GAIADR2_OUTPUT=# 2.088 5557554537690496 043.98073901875 +05.59010086212 9.3555 9.0763 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 20473_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20473_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20475_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20475_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20476_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20476_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20480_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20480_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20481_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20481_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20484_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20484_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20488_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20488_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20492_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20492_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:38.17 +05:29:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 1.449 5552331857465216 043.90924589994 +05.49615301908 9.5391 9.2012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20493_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20493_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20494_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20494_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:07.19 +07:55:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 5.468 8367803179074816 044.03145912305 +07.92235473987 9.6173 8.9595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20499_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20499_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20501_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20501_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:10.65 +08:34:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 0.810 8837977543281536 044.29451639528 +08.57131508646 9.7474 9.0574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20506_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20506_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:07.23 +03:12:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.01, MAG_FAINT_SEARCH_LIMIT=11.99)GAIADR2_OUTPUT=# 3.540 1614048710332416 044.03108004753 +03.20368449945 9.8059 9.4768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20508_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20508_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:02.90 +01:30:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 5.704 407785670617600 044.26344359956 +01.50159084321 9.7456 9.3934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20509_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20509_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:49.41 +08:06:51.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.07, MAG_FAINT_SEARCH_LIMIT=12.05)
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Considering the candidate 20511_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20511_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:33.23 +05:27:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.157 5595281530430720 043.63824735450 +05.46646564412 9.6756 9.1951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20513_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20513_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:07.33 +10:48:16.9 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 20515_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20515_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20516_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20516_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20520_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20520_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20523_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20523_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20525_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20525_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:33.16 +02:36:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 4.641 1555675809991936 043.63929495263 +02.61420759853 9.8601 9.4350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20527_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20527_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20528_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20528_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20529_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20529_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20530_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20530_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:59.10 +06:07:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 5.664 7137140430003712 043.99782918068 +06.12515727404 10.1896 9.7726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20531_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20531_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20532_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20532_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20533_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20533_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:49:27.33 +06:04:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 5.239 3276573517250248192 057.36531826742 +06.07787058407 10.6609 9.3271 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20534_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20534_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20535_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20535_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20538_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20538_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20539_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20539_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20540_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20540_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:22.13 +10:53:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 3.508 27354582284015104 044.84259072302 +10.88632302951 10.0795 9.3991 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 20541_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20541_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20542_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 20542_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 20543_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20543_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20544_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20544_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:05.45 +07:34:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 4.030 8143983843299328 044.52381652977 +07.56997872931 10.3653 10.0234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20552_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20552_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 20554_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20554_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:14.65 +03:34:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.53, MAG_FAINT_SEARCH_LIMIT=12.51)GAIADR2_OUTPUT=# 4.938 2054746714162560 044.06231177869 +03.57974648889 10.5477 9.8926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20555_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20555_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:42.55 +06:42:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 5.754 8026817135505280 044.17890032658 +06.70362073201 10.4487 10.1401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20566_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20566_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:00.21 +10:14:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 5.340 27116327562916096 044.49962800426 +10.23538889898 10.2120 9.3755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.340#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20573_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20573_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:38.82 +07:10:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 2.951 8080070434651136 044.41257221834 +07.17869817557 10.4554 10.0517 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20576_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20576_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:18.26 +10:44:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 2.310 27348706769112576 044.82604416730 +10.73769268377 10.3203 9.5292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20577_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20577_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:46.22 +10:57:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 2.887 27368047006304000 044.69275497804 +10.95054936264 10.2720 9.4925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20586_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20586_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:16.63 +09:45:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.854 21069876899133568 044.06869495133 +09.76564269610 10.3918 9.8954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20587_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20587_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:43.34 +06:06:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)GAIADR2_OUTPUT=# 5.569 7884018062842752 043.68212079027 +06.11562537617 10.4807 10.0181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20590_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20590_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:06.47 +02:47:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.580 1565257881365120 043.77732905831 +02.78940222169 10.5754 10.1475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20614_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20614_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:33:54.05 +06:05:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.017 3276229812490586240 053.47520773684 +06.08760653177 12.4149 11.9138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20617_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20617_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:41:23.67 +05:09:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.420 3274951698942135808 055.34873735738 +05.15961680765 12.3729 11.8680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20635_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20635_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:41:21.20 +07:44:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.466 3277962814614439424 055.33846130575 +07.74236274232 12.3925 11.8220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20639_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20639_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:42:56.24 +05:12:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.963 3274943452604926976 055.73460165601 +05.20207052116 12.3044 11.5607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20642_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20642_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:42:16.55 +06:43:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.590 3277638939720615296 055.56912268799 +06.72087510985 12.4208 11.8658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20644_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 20644_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:42:08.60 +06:55:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.839 3277662063824351232 055.53587793563 +06.91858982158 12.3669 11.7514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03071_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 03071_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04618_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 04618_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01133_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 01133_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 81s
Prepared the HTML report for the field Tau-07-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 ####
03:23:35.75 +09:23:52.0
03:29:25.82 +06:19:09.0
03:23:43.97 +03:53:23.5
03:03:15.85 +02:54:13.0
03:08:49.45 +10:59:39.3
03:05:03.70 +01:54:25.8
03:01:59.53 +03:47:58.8
03:08:30.43 +10:26:48.3
03:02:29.86 +05:35:05.8
03:03:01.41 +03:55:34.9
02:55:44.35 +07:16:52.7
02:55:31.51 +06:18:23.6
02:59:29.95 +06:20:18.8
02:55:17.13 +08:08:18.0
03:00:34.21 +10:48:04.6
02:58:12.40 +03:49:34.6
02:56:21.01 +06:33:59.0
03:03:06.96 +10:06:04.1
02:55:27.55 +06:57:40.4
03:43:43.72 +06:55:30.5
02:57:55.29 +08:10:18.8
02:59:59.96 +07:06:07.6
02:56:37.16 +01:45:05.7
02:57:00.74 +05:31:44.8
02:57:54.12 +07:26:05.2
02:56:18.34 +09:18:07.9
03:01:24.55 +07:10:56.7
02:57:29.66 +02:53:42.5
02:57:22.15 +05:20:42.6
02:55:57.77 +04:06:13.8
02:59:10.44 +08:56:21.6
02:55:25.57 +06:20:17.5
03:03:53.64 +09:45:11.1
02:56:14.93 +09:21:05.1
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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
SExtractor catalog cache: saved Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat to cache
SExtractor catalog cache: saved Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
Creating symlink local_wcs_cache/wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
Creating symlink local_wcs_cache/wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
Creating symlink local_wcs_cache/wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits exists and is non-empty
wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits exists and is non-empty
wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits exists and is non-empty
wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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 03:25:27.563 +05:58:50.42
Second-epoch image center 03:25:34.852 +06:00:24.35
Angular distance between the image centers 0.04 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 03:25:27.563 +05:58:50.42
Second-epoch image center 03:25:32.016 +06:00:04.69
Angular distance between the image centers 0.03 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 03:25:34.852 +06:00:24.35
Second-epoch second image center 03:25:32.016 +06:00:04.69
Angular distance between the image centers 0.01296 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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits &> /tmp/tmp.DPnbrpSAHy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits &> /tmp/tmp.cqiV7v0gVK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits &> /tmp/tmp.NokgLj4Jzh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits &> /tmp/tmp.NBk3iC64s2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits and wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits and wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat
Found non-empty wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits and wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat
The reference image (wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits) and catalog (wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat) found
'wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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 3762 out of 39596 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.836374
a=0.000000 b=1.000000 c=22.836374
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 696 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
1.9 pix Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
3.5 pix Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
3.5 pix Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
Limiting magnitude estimates:
15.5 mag. Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
15.5 mag. Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
14.7 mag. Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
14.7 mag. Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 13.9 (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.DPnbrpSAHy (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/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits' -> 'wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
WCS_IMAGE_NAME=wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
WCS-calibrated image found: wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
Checking if the catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits alredy exist and is non-empty...
Catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits
WCS catalog name: wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1675, passed=39589
Got 39589 stars (including 37839 good ones) from the SExtractor catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat
util/solve_plate_with_UCAC5 got 39589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 966 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits -region wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-31-17_20.00sec_-15.00C_LIGHT_0244.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.cqiV7v0gVK (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/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits' -> 'wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
WCS_IMAGE_NAME=wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
WCS-calibrated image found: wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
Checking if the catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits alredy exist and is non-empty...
Catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits
WCS catalog name: wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1671, passed=39536
Got 39536 stars (including 37792 good ones) from the SExtractor catalog wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat
util/solve_plate_with_UCAC5 got 39536 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 965 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits -region wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-07-Q2b1x1_2025-12-22_23-32-13_20.00sec_-15.00C_LIGHT_0245.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.NokgLj4Jzh (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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
WCS_IMAGE_NAME=wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
WCS-calibrated image found: wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
Checking if the catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits alredy exist and is non-empty...
Catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits
WCS catalog name: wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=48, blended=2574, passed=21322
Got 21322 stars (including 18734 good ones) from the SExtractor catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat
util/solve_plate_with_UCAC5 got 21322 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 970 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits -region wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-39-25_20.00sec_-14.90C_LIGHT_0084.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.NBk3iC64s2 (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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
WCS_IMAGE_NAME=wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
WCS-calibrated image found: wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
Checking if the catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits alredy exist and is non-empty...
Catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat corresponding to the image wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits
WCS catalog name: wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=48, blended=2617, passed=21230
Got 21230 stars (including 18594 good ones) from the SExtractor catalog wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat
util/solve_plate_with_UCAC5 got 21230 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 969 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Tau-07-Q2b1x1_214451_TTUQ2b1x1_14471_uh7brme8/Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits -region wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085.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 Tau-07-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__out50035.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out52879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52880.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out52884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52885.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out52908.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out53047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53689.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54181.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54395.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52997.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53121.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53126.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53288.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53946.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out54065.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out54278.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out13771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52871.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52980.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53241.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53487.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53508.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53544.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53552.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53591.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53600.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53602.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53648.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53653.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53770.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53857.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54063.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54244.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54321.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54398.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54408.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54522.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54534.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54750.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 409s
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: 150s
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Considering the candidate 52817_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52817_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:14:41.87 +01:16:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 3.146 3267000035145600640 048.67520901362 +01.28108647309 13.4292 12.8478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52823_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52823_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:19:35.25 +01:37:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 2.794 3267780035566354432 049.89622365426 +01.62795014381 13.5186 12.7890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52825_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52825_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:30.12 +04:51:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.153 3755141446664448 045.12489990990 +04.85826218201 12.5600 12.0775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52826_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52826_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 52827_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52827_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52829_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52829_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52830_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52830_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:16.32 +03:27:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.582 2621304440594432 046.56785164865 +03.45087944136 12.8451 12.3221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52832_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52832_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:08.97 +02:31:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.771 911082822587008 046.03751969368 +02.52961964598 12.5944 11.9689 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52834_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52834_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 52836_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52836_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 52837_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52837_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:07:03.56 +04:21:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.908 3445903801194880 046.76521595531 +04.35259026013 13.0125 12.4731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52838_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52838_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 52839_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52839_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:00.13 +02:48:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.984 978908946116992 045.75063502024 +02.80156257134 12.7401 12.0923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52840_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52840_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:25.36 +04:37:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.170 3514898156105472 046.35682393366 +04.63206115539 12.9415 12.3897 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 52842_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52842_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:01.87 +04:58:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.239 6762202669326208 045.00744671483 +04.96707661134 12.4735 11.9337 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52843_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52843_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:15.94 +01:28:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.296 3267205948762221056 047.06760499940 +01.46825140672 12.9922 12.4757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52844_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52844_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:03.32 +02:33:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.358 991141012979968 046.26421056172 +02.55939878206 12.6673 11.9674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52845_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52845_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:09.86 +03:10:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.801 1756714639121408 045.29111457603 +03.17983128557 12.6222 12.1125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52846_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52846_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:18:01.11 +04:28:40.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 52847_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52847_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:59.50 +05:37:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.996 6903803446777600 045.74822095264 +05.62676997565 12.7976 12.2722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52849_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52849_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52850_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52850_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:18:53.62 +01:21:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 5.025 3267766424814555648 049.72481208672 +01.36367656243 13.3994 12.8216 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52851_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52851_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:55.67 +09:02:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 5.268 14728954686570240 045.98337803844 +09.04466386460 12.4418 11.8486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52852_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52852_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:53.14 +04:08:24.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 52853_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52853_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:12.85 +05:04:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.556 6778076868450816 044.80337967636 +05.06765450858 12.5392 12.0203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52854_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52854_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:29.68 +03:50:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.644 3399964831297024 046.12325734042 +03.84181505852 12.7552 12.1800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52856_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52856_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:37.17 +02:52:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.867 1402564520196608 044.40485595131 +02.86700985930 12.0836 11.5665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52860_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52860_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:11:35.37 +02:03:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.855 3267339956037340160 047.89756971046 +02.05780279085 13.0737 12.5680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52862_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52862_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52863_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52863_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:31.55 +01:29:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.007 583531437053696 046.38149720670 +01.49780480024 12.3848 11.8336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52864_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52864_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:30.71 +01:43:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.348 502137512125056 044.87843858304 +01.71869750561 12.0969 11.6071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52865_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52865_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:49.30 +01:29:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.597 577449763362688 046.45638878310 +01.49357282413 12.4155 11.7645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52866_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52866_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:32.84 +08:47:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.774 14709335275966848 046.13729213743 +08.78449917246 12.4746 11.8871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52870_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52870_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:25.94 +01:35:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 4.032 459149183944320 045.35917239670 +01.59501429695 12.4506 11.8482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52871_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52871_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52872_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52872_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:21.58 +02:51:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.456 1764647443263232 044.59025252214 +02.85359413476 12.2478 11.7097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52873_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52873_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52875_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52875_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:37.00 +04:16:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 5.486 5209623531825024 044.40568597291 +04.27666319732 12.1895 11.6557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52876_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52876_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:07:56.64 +02:32:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 1.101 814948570272000 046.98592955021 +02.54224201454 13.0182 12.4961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52877_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52877_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:51.84 +03:55:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.612 2091580354222080 044.46645480878 +03.92245047510 12.1950 11.6142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52878_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52878_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:59.67 +01:53:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.235 650498567243776 046.24877248213 +01.89649586655 12.4579 11.9485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.235#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52879_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52879_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:09.19 +02:26:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.857 930637809250304 045.53764095816 +02.44329495366 12.4117 11.9557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52880_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52880_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:11.99 +02:34:06.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 52882_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52882_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:38.73 +05:03:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 3.382 3787851917597696 045.41219705842 +05.06209490030 12.2868 11.8071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52883_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52883_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:45.28 +03:10:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 1.764 1792758004621056 044.68819268767 +03.18101140188 12.2115 11.6415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52884_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52884_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:42.92 +08:07:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 1.741 8608939822930176 045.42927454237 +08.12465332312 12.1668 11.4838 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 52885_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52885_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:09.02 +03:02:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 3.359 1071508441007360 046.28813625063 +03.03602568117 12.5518 12.0541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52886_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52886_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:43.76 +02:18:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.201 932901256951424 045.18277610640 +02.30307696850 12.2703 11.7935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52888_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52888_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:22:09.74 +01:32:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.925 3267805633571349248 050.54160982015 +01.54471472343 13.4498 12.8672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52889_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52889_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:30.17 +06:36:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 4.664 7260972927032064 044.87684171596 +06.61475215518 12.2749 11.7012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52890_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52890_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:28.11 +01:23:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.480 244538258230528 045.36710128609 +01.39653559449 12.1314 11.5832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52891_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52891_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:09:44.95 +10:58:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.197 15549572613574400 047.43808446282 +10.97868361129 12.2952 11.7319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52892_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52892_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:41.22 +04:34:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.428 2247436126938624 044.92174107270 +04.58203560059 12.2387 11.6481 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 52893_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52893_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:32.64 +04:11:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.519 5117165771011712 044.13520056875 +04.19410090440 11.9095 11.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52894_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52894_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:09:22.77 +10:56:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 4.695 15548232583825536 047.34573869963 +10.94067584143 12.0602 11.4367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52895_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52895_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:43.20 +02:56:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 5.137 1778425698347392 044.42940097053 +02.94535101746 12.1234 11.5961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.137#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52896_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52896_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:25.64 +02:06:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 2.527 549137338705024 044.85748885722 +02.11544214361 12.0761 11.5502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52897_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52897_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 52898_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52898_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:36.87 +02:13:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.528 1303986431318784 044.65321671916 +02.22604991093 11.9021 11.3299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52899_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52899_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:21.84 +06:50:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.908 7422772934964224 046.09180936916 +06.83613659452 12.6178 12.1053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52900_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52900_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:49.56 +02:26:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.076 939227743820544 045.20593417961 +02.43569738920 12.0929 11.4418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52901_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52901_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:33.11 +03:16:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.073 1983965653133952 044.38926190563 +03.26787599539 12.0374 11.4460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52902_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52902_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:33.79 +04:00:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.261 2142226608068224 044.89095033583 +04.00013197861 12.1284 11.6246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52903_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52903_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:34.40 +02:09:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.011 1283477962613120 044.39377856572 +02.16008790231 11.8676 11.1565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52904_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52904_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:26:57.41 +08:12:49.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)
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Considering the candidate 52906_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52906_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:59.45 +03:45:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.009 3381651090748032 046.49730964964 +03.76305290561 12.6656 12.1465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52907_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52907_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:23.60 +03:21:00.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 5.332 1900475784529280 045.34965529402 +03.34957754210 12.5740 12.0713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52908_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52908_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:32.40 +03:18:40.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
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Considering the candidate 52909_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52909_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 52910_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52910_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:40.77 +02:46:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 2.119 1010936517902720 046.16960610534 +02.77750404229 12.4599 11.9231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52912_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52912_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52913_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52913_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:07.84 +01:52:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.346 623736626265984 046.53310256246 +01.86934871259 12.3792 11.8235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52914_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52914_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:23.22 +03:26:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.588 2621270080856320 046.59663177626 +03.44758513504 12.5933 12.0640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52917_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52917_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52918_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52918_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:58.65 +03:27:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 5.370 1827491405220352 044.99298354682 +03.46048352196 12.0977 11.5627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52919_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52919_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:08.29 +02:51:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.085 1017494932301056 046.28438021056 +02.85040829835 12.3685 11.8777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.085#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52920_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52920_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:03.50 +01:23:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.653 567038762640256 046.51384963141 +01.39506877470 12.3004 11.7490 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52921_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52921_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52922_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52922_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:10.92 +02:03:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.066 679296323199872 046.54578996796 +02.05336595288 12.3740 11.8155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52923_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52923_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:17.69 +07:42:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.273 8525063408748416 044.82405996629 +07.71386652054 11.9207 11.1519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52924_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52924_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:28.63 +02:05:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.197 549068619228416 044.86997495109 +02.09157109134 11.9747 11.4350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.197#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52925_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52925_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52926_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52926_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:39.65 +09:02:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.069 14731806544850048 045.91558885895 +09.03576252405 11.8681 11.3001 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 52927_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52927_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:59.31 +07:44:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.366 8499499760858368 045.24775811731 +07.73360932190 12.1126 11.4832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52928_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52928_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:08.74 +05:31:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.175 6857791461422080 044.53618134884 +05.51933183508 12.0177 11.5403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52929_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52929_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:19.55 +04:54:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.305 5273502580512256 044.58105337106 +04.90373549718 11.9274 11.3949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52930_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52930_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52932_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52932_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:25.71 +02:12:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.745 882946492455168 046.10715596420 +02.21476758667 12.1846 11.6802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52934_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52934_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:26.87 +02:36:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.863 994817504983808 046.61186996222 +02.61465276319 12.2575 11.7806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52935_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52935_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:57.48 +09:59:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.441 15084788432631680 046.23916068743 +09.98625704877 12.2786 11.7348 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 52936_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52936_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:18.90 +07:20:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.267 8131373819333888 044.32993457309 +07.34373913960 11.6052 10.8605 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 52937_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52937_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:39.30 +04:45:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.721 5250958296788992 044.66310933451 +04.75167882795 11.8624 11.2852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52939_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52939_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:32.24 +06:40:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.856 7240219645079552 045.38477940516 +06.67943583737 12.2232 11.7220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52940_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52940_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:21.00 +07:56:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.255 8567428963605888 044.83861358765 +07.94696415692 11.8345 11.2547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52941_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52941_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:12.88 +03:34:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.440 2025820110126208 044.55395295308 +03.57283102432 11.8957 11.2478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52942_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52942_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:04.76 +05:45:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 4.884 6888272844922624 045.02113272503 +05.75839461938 12.0713 11.5413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52943_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52943_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:24.49 +04:39:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.132 5247934639815936 044.60144151683 +04.66149281453 11.9790 11.4615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52944_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52944_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:20.93 +06:23:17.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 52945_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52945_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:31.57 +07:48:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.294 8492219791713408 045.63120855723 +07.81358703117 12.2684 11.7410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.294#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52946_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52946_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:08.99 +02:14:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.844 920123729319808 045.28745881637 +02.24770669059 11.9914 11.4300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52947_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52947_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:19.16 +07:15:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.657 7660709827577472 045.83028100737 +07.26076009401 12.1198 11.4975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52948_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52948_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:58.17 +01:42:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.007 3267309959985732224 047.24169619542 +01.70392335073 12.3864 11.7113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52950_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52950_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:05.46 +03:27:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 1.460 1908855265056896 045.52256519238 +03.45944438565 12.1007 11.6872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52952_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52952_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:07.27 +04:55:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.543 6758766695490176 045.03012362332 +04.91636357852 12.1179 11.6387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52953_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52953_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:08.90 +04:21:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.528 3676869962923776 045.53643306793 +04.35979732773 12.0984 11.4052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52954_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52954_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52955_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52955_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:29.03 +03:04:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.935 1786946913754368 044.62079434691 +03.06764586319 11.9118 11.2584 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 52956_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52956_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:19:38.25 +06:34:31.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)
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Considering the candidate 52957_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52957_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:58.55 +02:33:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.037 912182334213504 045.99352810982 +02.56041285357 12.4155 11.9103 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 52958_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52958_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:11.21 +02:11:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.942 881327289147904 046.04645658033 +02.18682830810 12.3755 11.8851 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52959_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52959_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 52960_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52960_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:36.31 +08:53:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 5.279 14724900237438464 045.90271909007 +08.89329228099 12.1603 11.5968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52961_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52961_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:17.47 +04:10:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.109 2204799987486208 044.32254566241 +04.17244974162 11.9473 11.4582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52962_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52962_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52963_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52963_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52964_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52964_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:23.09 +04:43:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 5.392 5250653354504320 044.59489300315 +04.72546960996 11.7767 11.3111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52966_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52966_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:54.64 +05:06:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.606 6767940745644928 045.22745101411 +05.10344230063 12.0174 11.3570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52967_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52967_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:22.14 +06:32:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 0.224 7234992669479936 045.09218742630 +06.54436313883 11.9915 11.4594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52968_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52968_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:25.36 +03:25:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.989 1902125051967744 045.35488610371 +03.42118530801 11.9396 11.3199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52969_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52969_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:36.58 +04:22:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.753 5135818813681024 043.90151843245 +04.37653332773 11.4727 10.7635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52970_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52970_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:12:27.47 +09:24:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.089 14430544654468736 048.11477465062 +09.41000630136 12.5859 12.0152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52971_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52971_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:19.15 +04:25:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.074 3669551338649984 045.82971537575 +04.42537166996 12.3625 11.8602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52972_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52972_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:45.36 +05:02:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.533 6775366744708224 044.93889400965 +05.04220165243 11.9924 11.4418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52973_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52973_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:56.60 +05:50:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.336 6972454203995520 045.23548489052 +05.84824293298 11.9924 11.3476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52974_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52974_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:52.14 +03:58:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.691 2106698638563968 044.21706801985 +03.97344155467 11.6334 10.9187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52975_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52975_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:34.14 +03:18:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 3.873 1991597810689664 044.14278279028 +03.30089807866 11.6137 11.0559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52976_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52976_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:15.26 +02:05:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.698 858551078197376 045.81411498897 +02.09255638117 12.0904 11.6135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52977_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52977_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:12.98 +05:28:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.830 6842501377883264 044.80396275045 +05.47144190569 11.8462 11.3590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52978_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52978_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52980_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52980_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52981_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52981_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:57.36 +06:59:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.507 7639544228746624 045.98966596118 +06.98972506799 12.2849 11.7430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52982_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52982_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52983_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52983_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:10:51.52 +09:15:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.048 14058772285228160 047.71490151493 +09.26295273161 12.3259 11.7719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52984_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52984_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:26.51 +02:22:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.166 891257253530752 046.36013314618 +02.38133371275 12.0674 11.5877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52985_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 52985_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 52986_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52986_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:21.77 +06:28:41.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 52987_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52987_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:56.97 +09:22:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 4.895 14945524117414528 045.73837017672 +09.37775402083 11.6936 11.1389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52988_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52988_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 52989_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52989_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 52990_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52990_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:17.27 +10:35:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.066 15181579815585408 046.57279193510 +10.59729577469 12.0516 11.5206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52991_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52991_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:57.18 +04:38:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 2.206 3703189522229760 046.23862133497 +04.64434491694 12.1836 11.6153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52992_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52992_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:56.50 +03:33:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.602 1864393763604480 045.73501073913 +03.55406582748 12.0063 11.4815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52993_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52993_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:07:35.87 +09:59:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.677 14908724837613952 046.89900813989 +09.98994866280 11.9376 11.4334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52994_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52994_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:31.97 +09:44:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.603 14879897017565696 046.63277215629 +09.74249489320 11.8910 11.2764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52995_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52995_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:11:18.36 +11:01:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.026 15629287206694400 047.82567331183 +11.02352536578 12.1689 11.5945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52996_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52996_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:11.98 +06:34:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.607 7233450776627968 045.29946999303 +06.58332739405 11.8807 11.3566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52997_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52997_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:46.34 +04:04:28.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
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Considering the candidate 52998_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52998_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:34.66 +05:41:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.367 7072063085593984 044.64367761690 +05.68460571427 11.6462 11.0943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52999_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 52999_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:38.90 +05:05:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.453 6776942997084160 044.91177853671 +05.09915081772 11.7834 11.0875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53000_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53000_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:16.06 +05:47:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.277 6933181023068160 046.06713160150 +05.79246699838 12.1942 11.7428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53001_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53001_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:55.48 +10:37:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 3.599 15190715210401536 046.23106882875 +10.62528278679 11.9637 11.3866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53003_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53003_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53004_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53004_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53005_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53005_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:26.11 +03:11:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.508 1757466258323968 045.35839302115 +03.18890062122 11.8543 11.1733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53006_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53006_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:27.55 +06:50:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.905 7247637053196544 045.36531502369 +06.84589939334 11.9894 11.4815 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53007_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53007_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:30.47 +05:57:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.217 7080683084193920 044.62694920178 +05.95949526252 11.6224 10.8951 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 53008_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53008_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:59.41 +05:59:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 4.516 6987641208320640 045.24637234839 +05.99269601629 11.8059 11.3036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53010_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53010_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:24.47 +10:23:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.141 15488133105725696 047.10283864127 +10.39716948230 12.0487 11.4928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53011_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53011_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:24.53 +09:37:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.438 14977890990953088 045.85247961589 +09.62792543876 11.9259 11.4008 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 53012_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53012_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:07:22.72 +10:52:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.697 15566851266691968 046.84481354650 +10.87450441970 11.8753 11.3253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53013_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53013_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:58.78 +01:42:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.901 643012439502208 046.24541553956 +01.71402062740 11.8655 11.4644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53014_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53014_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:25.66 +03:15:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.840 1840410666234112 045.85612855371 +03.25905305558 12.0922 11.5868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53015_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53015_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:03.22 +04:38:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 0.867 3699753548420096 046.01365740413 +04.64942525336 12.1293 11.5264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53016_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53016_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:52.08 +02:11:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.846 695887781621376 046.46663219188 +02.18433672402 11.9670 11.5021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53017_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53017_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:26.01 +04:45:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 0.424 3738240750762112 045.35836566351 +04.76246589885 11.7819 11.1833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53018_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53018_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:45.77 +03:46:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 0.993 1897585270861824 045.94056635202 +03.77681898381 12.0158 11.5169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53019_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53019_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:54.77 +11:02:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 5.030 15596950397495424 047.22862274086 +11.04546880117 11.8368 11.2684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53020_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53020_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:09.29 +10:48:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.592 15574444768874240 046.53886639805 +10.81440809722 11.8214 11.2675 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 53021_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53021_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:00.34 +02:18:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.377 878067409582464 045.75165195659 +02.30717034873 11.9595 11.4530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53022_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53022_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:54.50 +07:12:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.873 7656487875374976 045.97757330164 +07.20365734544 11.9373 11.3017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53023_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53023_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:20.55 +07:52:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.392 7836734767737600 045.83533073004 +07.87938500245 11.8615 11.2413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53024_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53024_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:35.79 +01:51:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.703 484541030591872 045.39904417426 +01.86272833707 11.7215 11.2209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53026_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53026_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53027_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53027_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:42.05 +02:08:15.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 2.945 693860557058688 046.17439925545 +02.13754248710 11.8327 11.3254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53028_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53028_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53029_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53029_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:10.67 +05:05:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.501 3870349649266944 046.04475796821 +05.09676320575 12.1044 11.6017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53031_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53031_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:14.25 +02:05:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.585 691936411710976 046.05932092221 +02.09181316032 11.7533 11.3058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53032_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53032_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:14.27 +01:21:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.932 565943546370432 046.55966519209 +01.35388401761 11.8824 11.2974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53033_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53033_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:24.39 +05:56:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.572 6975168623320704 045.35136698854 +05.94470216685 11.7806 11.2999 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 53034_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53034_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53035_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53035_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:54.33 +07:24:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.081 7724378423062784 045.47722605050 +07.40164232623 11.8759 11.3212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53036_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53036_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 53037_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53037_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:07:53.14 +01:22:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.567 3267203371781846144 046.97051688667 +01.38152920057 11.8599 11.3103 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 53038_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53038_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:53.11 +07:10:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 3.415 7658373365661568 045.72192154722 +07.16884180889 11.9755 11.4602 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53039_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53039_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:25.40 +09:05:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 1.348 14697103209101824 046.60617335804 +09.08364002305 11.9058 11.2823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53040_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53040_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:41.08 +04:55:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.369 5272433133263872 044.67108634930 +04.92846360321 11.5149 11.0301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53041_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53041_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53042_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53042_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:36.36 +08:49:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.773 14665256027127168 046.40128670933 +08.82541738092 11.9218 11.3713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53043_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53043_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:09:09.39 +10:33:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 4.842 15497036573635200 047.28777457461 +10.56388308455 11.7757 11.2454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53044_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53044_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:01.95 +05:02:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.228 3784278504807936 045.50700749426 +05.04126475336 11.8308 11.2883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53045_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53045_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:01.26 +02:58:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 5.752 1744310773578880 045.25391830154 +02.96644799793 11.5473 11.0512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53046_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53046_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:24.77 +10:29:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 0.496 15176838171693312 046.60313092377 +10.49189259603 11.7301 11.2076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53047_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53047_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:24.57 +05:41:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.835 6917199449047808 045.60224805037 +05.68670051838 11.8175 11.1519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53048_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53048_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:28.64 +09:43:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 2.730 15028575900626048 045.61863758004 +09.72750983130 11.4739 10.9204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53049_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53049_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53050_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53050_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 53051_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53051_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53052_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53052_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53053_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53053_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53054_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53054_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:01.71 +04:15:55.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)
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Considering the candidate 53055_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53055_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:15.19 +08:51:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.059 14669138677588608 046.31243893958 +08.85113961387 11.7551 11.2415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53056_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53056_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:35.85 +05:20:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.317 6837076834768768 044.89875994436 +05.34178163250 11.5554 11.1280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53057_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53057_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:03.76 +01:46:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.225 645516404728064 046.26556688766 +01.78086214649 11.6565 11.2351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53058_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53058_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:39.33 +06:05:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.940 6957331623447040 045.91343316910 +06.08379902407 11.8448 11.3766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53059_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53059_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53060_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53060_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53061_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53061_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53062_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53062_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:43.80 +01:49:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.722 668674868386304 046.43183988488 +01.82522742304 11.7554 11.2991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53063_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53063_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:52.54 +06:23:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 2.703 7344497155417344 046.21833499662 +06.38577078136 11.7400 11.2804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53064_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53064_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53066_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53066_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:04.86 +09:13:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.611 14760810459480832 046.27038094790 +09.22330685729 11.4629 11.2103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53067_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53067_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:25.99 +05:01:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.020 3774863936329728 045.85729724962 +05.02029010057 11.7196 11.2398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53068_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53068_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:02.82 +07:25:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 4.374 7712975285212800 045.76063468638 +07.41814162570 11.6003 11.0817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53069_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53069_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:28.51 +04:36:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 5.550 5236355407987584 044.36732718301 +04.61408766325 11.3222 10.8080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53070_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53070_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:35.55 +05:07:35.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)
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Considering the candidate 53072_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53072_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53073_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53073_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 53074_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53074_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:01.77 +06:06:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.614 7005027235989376 045.75608643229 +06.10672311895 11.6668 11.1491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53075_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53075_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53076_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53076_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:07.50 +08:07:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 3.544 8576813467510912 045.03223309796 +08.13182472241 11.4049 10.8890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53077_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53077_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:55.08 +09:27:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.573 14807058667438208 047.22905749103 +09.46277036632 11.6484 11.1311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53078_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53078_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53079_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53079_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:18.88 +06:39:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.619 7414316143773312 045.82938728969 +06.65121354149 11.5219 11.0262 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 53080_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53080_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:06:35.32 +08:29:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.674 13893703807006976 046.64791511226 +08.49808813505 11.7456 11.2217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53081_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53081_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53082_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53082_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:15.68 +01:18:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.051 3267190559894829312 047.06533941844 +01.31623494253 11.6588 11.1849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53083_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53083_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53085_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53085_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:06.34 +03:42:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.104 1931193390573824 045.27608045481 +03.71524371023 11.3400 10.9032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53086_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53086_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53087_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53087_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:45.89 +04:12:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 3.339 2161197479573120 045.44028176771 +04.21294875948 11.3651 10.9186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53088_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53088_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:54.03 +05:40:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.411 6910705458496768 045.72389539527 +05.67478674927 11.6289 11.1377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53089_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53089_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:24.65 +04:43:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 5.361 3751572329306496 045.10134376938 +04.72917128295 11.5019 11.0575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53090_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53090_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53091_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53091_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53092_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53092_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 53093_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53093_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 53095_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53095_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:23.67 +06:11:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.121 6964963781036800 046.09875084941 +06.19671486973 11.4921 10.9493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53096_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53096_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:11:18.11 +10:51:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.977 15622067366378240 047.82534655798 +10.85283145937 11.4079 11.0167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53097_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53097_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53098_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53098_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 53099_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53099_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:56.75 +03:37:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 5.289 1886452715633920 045.98743296415 +03.63046216517 11.4006 10.9455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53100_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53100_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:05:21.94 +01:43:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 4.021 597412771015424 046.34073492005 +01.72208715533 11.3038 10.8201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53101_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53101_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53102_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53102_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 53103_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53103_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:01.45 +10:16:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 2.285 15110210343409920 047.00559824633 +10.27309999978 11.2760 10.7731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53104_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53104_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53105_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53105_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53106_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53106_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:03.52 +04:13:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 5.059 3472085922435456 045.76330377211 +04.22811523367 11.3145 10.8431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53107_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53107_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:38.20 +06:38:21.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)
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Considering the candidate 53108_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53108_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53109_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53109_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:16.73 +02:42:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 2.875 1055569818047488 046.06907852586 +02.70031367683 11.2707 10.8221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53110_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53110_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53111_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53111_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:27.50 +02:23:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 2.903 894113407389312 046.11377843963 +02.38613546902 10.9956 10.5754 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 53112_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53112_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53113_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53113_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:20.87 +02:26:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.005 906620352153984 046.08653198509 +02.43611344145 11.0520 10.5501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53114_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53114_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53115_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53115_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53117_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53117_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53118_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53118_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53120_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53120_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:09:39.12 +10:09:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 5.398 15289984790155136 047.41180413798 +10.16306795281 10.9136 10.4378 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 53121_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53121_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:15.50 +02:39:35.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)
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Considering the candidate 53122_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53122_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:22.21 +03:31:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 3.566 1911024224195328 045.59346661345 +03.52710906845 10.6352 10.1245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53123_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53123_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53124_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53124_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53125_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53125_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53126_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53126_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:15.28 +02:54:02.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)
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Considering the candidate 53127_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53127_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:08.66 +04:58:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 3.034 3727726670833664 046.03526093709 +04.97702508849 10.5118 10.0789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53128_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53128_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53129_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53129_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53130_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53130_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 53131_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53131_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53132_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53132_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:14:01.48 +10:49:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.08, MAG_FAINT_SEARCH_LIMIT=12.06)GAIADR2_OUTPUT=# 4.486 15446008066772224 048.50534722046 +10.82197903277 10.2333 9.7794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53133_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53133_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53134_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53134_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53135_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53135_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 53136_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53136_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53137_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53137_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 53140_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53140_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53141_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53141_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53142_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53142_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 53143_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53143_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53144_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53144_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 53146_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53146_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53148_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53148_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:22.60 +06:39:07.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53149_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53149_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:42.84 +08:54:29.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53151_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53151_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:44.23 +10:52:14.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53152_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53152_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:12.95 +08:22:54.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53153_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53153_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:31.06 +02:01:01.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53154_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53154_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:07.51 +03:29:09.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53156_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53156_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:24.57 +10:47:48.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53158_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53158_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:24.41 +10:12:15.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53161_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53161_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:04.12 +06:10:30.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53164_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53164_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:04.98 +10:39:24.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53165_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53165_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:09.20 +03:40:40.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53166_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53166_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:13.58 +04:02:52.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53167_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53167_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:14.82 +01:53:07.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53171_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53171_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:17.13 +10:12:37.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53174_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53174_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:43.84 +11:00:51.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53175_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53175_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:00.19 +10:09:40.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53180_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53180_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:40.29 +09:38:11.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53181_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53181_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:50.43 +10:30:09.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53184_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53184_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:20.86 +03:19:04.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53185_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53185_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:48.27 +10:51:01.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.83, MAG_FAINT_SEARCH_LIMIT=10.81)
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Considering the candidate 53186_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53186_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:46.14 +03:29:53.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53187_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53187_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:21.77 +06:14:50.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53188_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53188_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:19.45 +11:08:16.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53189_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53189_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:20.83 +05:28:40.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53191_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53191_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:50.25 +07:31:35.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53192_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53192_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:29.98 +10:07:30.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53193_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53193_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:08.04 +03:56:10.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53194_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53194_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:04.28 +07:39:11.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53195_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53195_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:28.18 +07:46:41.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53196_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53196_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53198_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53198_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:46.40 +03:34:05.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53199_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53199_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:47.66 +07:01:08.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53200_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53200_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:16.69 +05:59:49.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53201_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53201_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:56.95 +10:38:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.26, MAG_FAINT_SEARCH_LIMIT=11.24)GAIADR2_OUTPUT=# 1.502 27334687995840000 044.23696568813 +10.64526716186 8.5665 7.7853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53202_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53202_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:21.45 +10:28:51.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 53203_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53203_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:29.93 +06:20:20.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53206_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53206_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:44.24 +07:16:52.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53207_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53207_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53209_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53209_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:31.47 +06:18:23.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53215_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53215_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:12.38 +03:49:36.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53217_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53217_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:29.83 +05:35:05.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53218_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53218_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:34.13 +10:48:04.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53219_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53219_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:17.02 +08:08:17.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53221_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53221_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:55.15 +05:35:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.59, MAG_FAINT_SEARCH_LIMIT=11.57)GAIADR2_OUTPUT=# 3.872 5557554537690496 043.98073901875 +05.59010086212 9.3555 9.0763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.872#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53224_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53224_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:20.80 +06:33:58.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53226_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53226_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:07.09 +10:06:05.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53229_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53229_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53234_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53234_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:09.21 +10:32:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.65, MAG_FAINT_SEARCH_LIMIT=11.63)GAIADR2_OUTPUT=# 1.816 27329770258039296 044.28801227425 +10.54144020455 9.0116 8.2093 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 53237_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53237_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:59.73 +07:06:06.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53241_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53241_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53242_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53242_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:27.34 +06:57:39.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53243_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53243_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:38.44 +04:49:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.77, MAG_FAINT_SEARCH_LIMIT=11.75)GAIADR2_OUTPUT=# 1.949 5301677565937152 043.66070837587 +04.82690332679 9.3364 8.6517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53244_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53244_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:28.18 +05:12:36.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)
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Considering the candidate 53245_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53245_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53246_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53246_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53247_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53247_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:08:30.28 +10:26:49.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53248_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53248_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:53.93 +07:26:05.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53250_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53250_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:28.08 +09:34:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.81, MAG_FAINT_SEARCH_LIMIT=11.79)GAIADR2_OUTPUT=# 3.769 21051219561205120 044.11797774521 +09.58186951761 9.3390 8.3164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53251_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53251_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:38.06 +05:29:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.83, MAG_FAINT_SEARCH_LIMIT=11.81)GAIADR2_OUTPUT=# 2.596 5552331857465216 043.90924589994 +05.49615301908 9.5391 9.2012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53253_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53253_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:00.60 +05:31:43.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53262_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53262_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53264_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53264_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53268_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53268_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:37.30 +01:45:06.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53270_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53270_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53271_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53271_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:45.32 +06:20:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 0.635 7167308280279936 044.18865583522 +06.33707870444 9.7752 9.2255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53273_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53273_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53274_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53274_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:07.19 +07:55:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.99, MAG_FAINT_SEARCH_LIMIT=11.97)GAIADR2_OUTPUT=# 5.489 8367803179074816 044.03145912305 +07.92235473987 9.6173 8.9595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53276_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53276_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:07.17 +03:12:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.04, MAG_FAINT_SEARCH_LIMIT=12.02)GAIADR2_OUTPUT=# 4.677 1614048710332416 044.03108004753 +03.20368449945 9.8059 9.4768 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 53277_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53277_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53282_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53282_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53285_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53285_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:03.05 +01:30:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.10, MAG_FAINT_SEARCH_LIMIT=12.08)GAIADR2_OUTPUT=# 3.395 407785670617600 044.26344359956 +01.50159084321 9.7456 9.3934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53288_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53288_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:26.84 +07:46:50.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)
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Considering the candidate 53290_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53290_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53292_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53292_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:33.04 +05:27:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 3.470 5595281530430720 043.63824735450 +05.46646564412 9.6756 9.1951 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53295_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53295_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53296_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53296_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:17.98 +09:18:07.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53297_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53297_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53304_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53304_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:05.67 +10:47:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 4.120 27352108383210624 044.77439172733 +10.79430506908 9.7267 9.1119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53307_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53307_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:29.49 +02:53:41.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53308_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53308_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:07.23 +10:48:16.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.20, MAG_FAINT_SEARCH_LIMIT=12.18)
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Considering the candidate 53311_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53311_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53317_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53317_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53320_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53320_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53323_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53323_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53324_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53324_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53325_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53325_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53326_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53326_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53330_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53330_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53331_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53331_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53333_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53333_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:53.49 +09:45:15.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53337_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53337_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53343_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53343_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53344_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53344_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53345_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53345_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53347_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53347_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53353_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53353_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53354_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53354_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:02.66 +10:12:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 4.535 27106092656504960 044.75997282040 +10.20754289717 10.0974 9.2472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53358_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53358_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:25.29 +06:20:15.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53362_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53362_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53364_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53364_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53366_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53366_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53367_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53367_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:22.14 +10:53:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 3.360 27354582284015104 044.84259072302 +10.88632302951 10.0795 9.3991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53368_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53368_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:14.67 +09:21:04.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53369_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53369_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53370_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53370_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:56.97 +01:46:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 4.853 506222025490304 044.73840173638 +01.77154090790 10.4146 10.0160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53371_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53371_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53380_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53380_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53383_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53383_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53384_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53384_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53394_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53394_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53408_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53408_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53410_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53410_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53413_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53413_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53414_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53414_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53417_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53417_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:18.27 +10:44:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 2.126 27348706769112576 044.82604416730 +10.73769268377 10.3203 9.5292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53420_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53420_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53428_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53428_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:46.25 +10:57:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 2.727 27368047006304000 044.69275497804 +10.95054936264 10.2720 9.4925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53429_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53429_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53430_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53430_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53432_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53432_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:43.34 +10:32:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 1.710 27338433207344256 044.68101666211 +10.54931761990 10.4002 9.6070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53435_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53435_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 53438_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53438_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53442_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53442_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53448_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53448_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:06.43 +02:47:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.198 1565257881365120 043.77732905831 +02.78940222169 10.5754 10.1475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53455_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53455_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 53457_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53457_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53461_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53461_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53469_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53469_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53474_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53474_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53480_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53480_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53482_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53482_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53485_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53485_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53487_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53487_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53490_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53490_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53493_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53493_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53495_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53495_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53501_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53501_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:37.56 +02:39:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.786 1385629464730880 044.40720457002 +02.65257191422 10.7853 10.3574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53502_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53502_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53508_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53508_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53517_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53517_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53518_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53518_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53521_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53521_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:42.12 +05:25:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 3.379 5548002530437504 043.67575125075 +05.42415475966 10.7313 10.2128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53523_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53523_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:07.77 +05:30:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 5.395 5550235913427200 043.78368764085 +05.50853953660 10.7652 10.3542 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 53528_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53528_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53529_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53529_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53541_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53541_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:38.89 +03:05:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 2.733 1599759354299520 044.16271812036 +03.08712413072 10.9128 10.4994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53544_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53544_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53548_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53548_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53552_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53552_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53554_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53554_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:32.00 +09:22:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 4.043 20998477362844032 044.38438888733 +09.37852397622 10.8437 10.1099 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 53556_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53556_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:07.54 +02:23:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 5.877 1350719970564224 044.03273177009 +02.38741306296 10.8966 10.4987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53558_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53558_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53563_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53563_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53565_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53565_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53566_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53566_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:33.38 +02:52:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 4.107 1589520152274304 043.89013970141 +02.87843391425 10.8804 10.4430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53567_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53567_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:10.57 +06:17:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 4.706 7168820108768256 044.29534987947 +06.28627219018 10.9263 10.4511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.706#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53569_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53569_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:38.47 +05:47:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 4.392 7109240322463232 043.90912971867 +05.79155647693 10.8873 10.1525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53576_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53576_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:26.34 +10:18:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 5.715 15155397694908672 045.86106087494 +10.31001883317 11.0982 10.6161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53577_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53577_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53578_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53578_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53580_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53580_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:30.43 +05:55:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 3.642 7127171810206976 043.87780451364 +05.93339688483 10.9464 10.4251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53582_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53582_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53585_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53585_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53586_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53586_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53589_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53589_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:05.94 +02:11:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 5.075 1339278177695872 044.02606966548 +02.18497035817 10.9349 10.4343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53590_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53590_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53591_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53591_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53592_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53592_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53594_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53594_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53597_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53597_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53600_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53600_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53601_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53601_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53602_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53602_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53606_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53606_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53610_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53610_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53611_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53611_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:03.89 +01:47:31.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)
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Considering the candidate 53612_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53612_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53614_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53614_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:46.24 +02:16:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 4.636 1344015526010368 043.94370600687 +02.27928935546 10.8491 10.3403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53618_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53618_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 53624_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53624_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53631_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53631_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53634_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53634_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53638_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53638_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53639_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53639_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53641_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53641_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53642_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53642_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53648_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53648_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53650_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53650_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 53652_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53652_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:28.01 +11:03:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.462 27462471862817024 044.86712179597 +11.05976938921 10.9559 10.1932 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 53653_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53653_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53655_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53655_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53657_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53657_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53665_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53665_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53671_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53671_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53672_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53672_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53674_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53674_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53677_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53677_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53679_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53679_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:51.73 +05:29:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 3.138 5552228778248192 043.96509481223 +05.49783296475 11.2777 11.0061 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53681_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53681_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:54.12 +10:41:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 5.091 27195462336093184 045.72621272433 +10.68721577770 11.2912 10.8332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53687_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53687_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:52.77 +01:38:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 4.467 1164696347204480 043.96959279085 +01.64273615303 11.0841 10.6245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53689_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53689_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:37.98 +03:54:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 5.258 2181469725202304 044.65949243180 +03.90741161009 11.2408 10.6508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53693_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53693_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53695_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53695_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53703_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53703_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53718_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53718_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53719_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53719_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53722_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53722_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53723_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53723_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:17.09 +02:32:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 3.923 1375798284017536 044.32225192673 +02.53831720834 11.4429 11.0229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53728_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53728_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53738_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53738_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53747_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53747_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53750_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53750_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53756_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53756_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53758_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53758_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53760_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53760_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53761_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53761_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53768_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53768_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53769_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53769_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53770_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53770_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53771_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53771_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53774_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53774_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53783_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53783_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53786_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53786_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:57.40 +10:27:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 5.289 21320599910133504 043.98770434460 +10.46092140445 11.0034 10.1924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53793_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53793_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53802_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53802_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53805_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53805_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53807_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53807_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53809_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53809_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53812_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53812_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53826_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53826_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53828_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53828_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (17.9") between the two second-epoch detections
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Considering the candidate 53829_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53829_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53835_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53835_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53836_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53836_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:18.97 +02:05:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.879 1243758105176192 043.82904741242 +02.08888294417 11.4351 10.9071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53839_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53839_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53844_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53844_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53850_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53850_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53851_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53851_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:32.25 +10:57:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 3.005 27449513945872640 044.88513970085 +10.96196870581 11.4537 10.8217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53855_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53855_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:45.90 +01:27:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 4.069 445302209250560 044.69214910919 +01.45929652611 11.6203 11.1794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53857_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53857_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53858_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53858_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53867_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53867_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:11.44 +01:45:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.339 1174725095638144 044.04800117852 +01.76613015093 11.4795 11.0147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53868_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53868_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53871_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53871_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53880_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53880_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53881_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53881_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53882_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53882_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53884_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53884_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:00.26 +10:38:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.972 27340902813270016 044.75143525884 +10.64051966739 11.4761 10.6914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53889_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53889_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53893_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53893_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53894_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53894_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53897_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53897_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 53898_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53898_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53899_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53899_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53900_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53900_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53907_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53907_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 53918_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53918_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53932_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53932_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:44.30 +07:14:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.853 8108485937989504 044.18586925881 +07.24692521174 11.6143 11.1583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53935_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53935_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53944_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53944_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (18.9") between the two second-epoch detections
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Considering the candidate 53946_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53946_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:39.46 +07:45:02.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 53950_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53950_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53953_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53953_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53954_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53954_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:59.97 +02:57:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.933 1602916154610432 043.75013017953 +02.96228602854 11.6861 11.1646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53957_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53957_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53958_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53958_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 53961_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53961_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53963_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53963_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:20.43 +02:46:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.888 1564300104315008 043.83577621594 +02.77910838095 11.5910 11.0847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53968_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53968_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:48.63 +10:40:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.515 27236590942892160 045.45321136292 +10.66760505096 11.7694 11.2710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53969_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53969_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 53972_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53972_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:32.28 +05:38:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.203 5605555092189952 043.88393068157 +05.64887038371 11.6191 11.1439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53982_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 53982_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 53991_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 53991_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54004_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54004_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54007_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54007_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54009_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54009_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54013_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54013_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54016_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54016_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54018_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54018_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54022_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54022_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54026_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54026_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54029_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54029_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:31.37 +09:42:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.747 21078054516894976 044.37974883268 +09.71696264107 11.5918 11.0199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54030_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54030_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54031_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54031_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54036_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54036_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54045_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54045_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54046_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54046_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:04.33 +03:48:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 4.385 5074589759921024 043.51926231280 +03.80520416065 11.7516 11.2836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54053_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54053_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:57.12 +05:48:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 5.097 7110541696842240 043.98922356073 +05.80486004232 11.7306 11.2149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54059_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54059_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:35.76 +05:51:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.115 7112706360357760 043.89893190870 +05.85372184239 11.7267 11.2232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54060_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54060_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:13.47 +05:33:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.292 5556347651235584 043.80638085981 +05.55969170043 11.8598 11.4049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54063_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54063_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54065_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54065_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:00.02 +05:08:30.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 54075_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54075_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54084_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54084_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54089_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54089_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:19.08 +04:44:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 4.423 5242063419916544 044.32880133085 +04.73343225893 11.9460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54091_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54091_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54093_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54093_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54101_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54101_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54109_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54109_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:36.79 +02:12:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.231 1341958237290112 043.90446548884 +02.20400785268 11.5242 11.0399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54120_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54120_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54121_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54121_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:25.32 +09:41:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.214 21022250006694528 044.85501089094 +09.69888165177 11.8568 11.1262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54122_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54122_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54124_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54124_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:57.74 +09:45:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.439 15027506453153792 045.74183274602 +09.76198183733 12.0265 11.5108 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54126_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54126_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:35.51 +05:51:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.837 7112706360357760 043.89893190870 +05.85372184239 11.7267 11.2232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54130_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54130_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:00:07.56 +09:45:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.711 27025381631125504 045.03253390174 +09.75795987796 12.0758 11.5434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54136_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54136_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54143_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54143_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:43.36 +04:41:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.106 5287040317476480 044.17997679501 +04.68817340123 11.7941 11.0995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.106#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54146_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54146_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54152_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54152_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54153_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54153_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54158_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54158_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:34.37 +04:20:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.362 5133383567485312 043.89289207266 +04.33806890743 11.8834 11.3753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54163_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54163_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54165_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54165_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54166_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54166_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:22.05 +03:02:51.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 54169_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54169_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:57.95 +10:03:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.754 27097842023677952 044.49132686808 +10.05189141455 11.7660 11.1895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54171_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54171_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:50.60 +01:43:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.283 1168609062209280 043.96100014775 +01.72373155662 11.8313 11.2800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54173_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54173_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54174_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54174_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54179_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54179_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54181_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54181_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:53.81 +10:01:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.595 21092897923858944 044.47320846764 +10.02441629745 11.8064 11.2384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54184_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54184_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 54187_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54187_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:18.20 +02:35:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.757 1555190478029440 043.57603331779 +02.59553784855 11.7698 11.3299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54190_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54190_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54196_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54196_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54198_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54198_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:02:19.08 +10:26:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.175 27180923871562112 045.57934255415 +10.44131520132 12.3587 11.6818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54202_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54202_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54207_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54207_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:25.71 +06:48:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.073 8040900332624896 044.10797318935 +06.80394501466 11.9561 11.3221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54211_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54211_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:31.99 +10:27:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.701 27316369960076800 044.38459823370 +10.46278894572 11.7590 11.1857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54215_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54215_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54236_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54236_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:46.31 +06:33:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.901 7927959872628736 044.19403224845 +06.56224445052 11.8654 11.2584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54239_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54239_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:21.61 +01:52:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.144 1233102290555520 043.59086768731 +01.87554848027 11.9157 11.3782 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 54244_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54244_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54245_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54245_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54246_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54246_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54252_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54252_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54256_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54256_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54258_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54258_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:56.63 +03:07:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.977 1656448627480448 043.73592986216 +03.11903564959 12.0309 11.5091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54259_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54259_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:09.12 +02:11:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.259 1248637187992064 043.78754393758 +02.19362433031 11.6429 10.8380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54261_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54261_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:36.39 +05:45:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 5.245 5621463651020416 043.65036890073 +05.75530684138 11.7073 11.1493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54268_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54268_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:53.66 +10:01:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.459 21092897923858944 044.47320846764 +10.02441629745 11.8064 11.2384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54277_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54277_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:02.66 +04:18:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.697 5212273526769280 044.26089527792 +04.31118698323 12.0560 11.5047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.697#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54278_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54278_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:09.76 +01:47:57.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 54283_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54283_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54287_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54287_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:04:38.48 +10:01:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 1.791 15131929993637248 046.16081821444 +10.03033262422 12.0433 11.5235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54306_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54306_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:17.08 +10:58:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 0.424 27412409724012672 044.32111856496 +10.97650329050 11.7286 10.9712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54308_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54308_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54319_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54319_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54320_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54320_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54321_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54321_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54335_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54335_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54347_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54347_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54357_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54357_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54359_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54359_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:46.48 +01:39:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 4.666 419532406004608 044.19457437454 +01.66081445992 11.9791 11.5816 NOT_AVAILABLE#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 54362_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54362_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:49.99 +01:29:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 4.156 445547023045376 044.70939602195 +01.49811493384 12.1691 11.7386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54368_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54368_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:58:16.73 +01:47:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.980 513265771854592 044.56995881185 +01.79253233990 12.1160 11.5278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54374_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54374_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:54.46 +10:18:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.973 21314754459194752 043.97712368136 +10.30856657518 11.9541 11.2708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54383_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54383_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:17.07 +02:23:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 3.330 1351162351587072 044.07099862989 +02.39330574017 11.9013 11.4034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54390_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54390_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54391_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54391_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54395_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54395_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:01:21.24 +10:21:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.820 27088358735881984 045.33866036555 +10.36123258007 12.3180 11.6714 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 54397_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54397_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54398_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54398_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54405_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54405_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54408_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54408_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54409_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54409_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:03:42.73 +10:46:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 4.935 27217654431873280 045.92913414846 +10.76584153059 12.2652 11.7351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54418_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54418_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:23.06 +03:08:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.977 1612678615924864 044.09603404372 +03.14576694638 12.2321 11.6315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.977#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54432_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54432_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54445_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54445_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:39.62 +01:37:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.716 1154869462036864 043.66581434072 +01.61718820243 11.9889 11.4720 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54456_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54456_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
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Considering the candidate 54461_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54461_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54468_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54468_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:13.67 +04:01:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.070 5107545044246272 043.80780952413 +04.02781011392 12.1321 11.6407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54469_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54469_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:47.12 +04:23:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.219 5135234698128640 043.94694876934 +04.39242815278 12.0905 11.5534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54470_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54470_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54472_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54472_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54474_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54474_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54475_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54475_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:56:00.83 +05:26:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.118 5550923108193536 044.00287455338 +05.43625912875 12.1810 11.6221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54486_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54486_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:55:02.83 +01:53:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.857 1186991522234368 043.76146477660 +01.88779515022 11.8560 11.1324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.857#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54490_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54490_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54492_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54492_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54493_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54493_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54510_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54510_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54522_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54522_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54532_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54532_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54534_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54534_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54535_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54535_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:57:24.32 +01:55:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.785 1270039009814528 044.35098940007 +01.93013747801 12.1559 11.6523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54538_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54538_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54549_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54549_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54574_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54574_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54583_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54583_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54596_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54596_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:59:07.85 +01:45:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 5.672 503374462706688 044.78302034147 +01.75562778699 12.4458 11.8935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54625_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54625_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54629_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54629_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54639_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54639_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54644_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54644_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54661_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54661_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 02:54:10.00 +02:10:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 3.803 1259421850708224 043.54256322752 +02.17908768459 12.4212 11.9812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54663_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54663_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54712_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54712_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 54720_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54720_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54747_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54747_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54750_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 54750_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 54775_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54775_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54777_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54777_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 54846_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 54846_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 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 13771_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 13771_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 19147_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 19147_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 06374_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 06374_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:23:35.76 +09:23:52.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 15896_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 15896_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:43:43.72 +06:55:30.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 29266_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 29266_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 37544_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 37544_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:23:43.96 +03:53:23.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 14958_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 14958_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 50035_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 50035_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:40:42.76 +07:09:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.307 3277714466722036096 055.17797186303 +07.16460918181 12.6026 12.0152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 16775_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
Preparing report for the candidate 16775_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
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Considering the candidate 18119_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085
The candidate 18119_Tau-07-Q2b1x1_2026-02-21_21-40-14_20.00sec_-14.90C_LIGHT_0085 did not pass the final checks
**** FOUND 03:29:25.84 +06:19:09.0 in the exclusion list exclusion_list_local.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 17s
make_report_in_HTML.sh TOTAL: 576s
Prepared the HTML report for the field Tau-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:23:35.75 +09:23:52.0
03:29:25.82 +06:19:09.0
03:23:43.97 +03:53:23.5
03:03:15.85 +02:54:13.0
03:08:49.45 +10:59:39.3
03:05:03.70 +01:54:25.8
03:01:59.53 +03:47:58.8
03:08:30.43 +10:26:48.3
03:02:29.86 +05:35:05.8
03:03:01.41 +03:55:34.9
02:55:44.35 +07:16:52.7
02:55:31.51 +06:18:23.6
02:59:29.95 +06:20:18.8
02:55:17.13 +08:08:18.0
03:00:34.21 +10:48:04.6
02:58:12.40 +03:49:34.6
02:56:21.01 +06:33:59.0
03:03:06.96 +10:06:04.1
02:55:27.55 +06:57:40.4
03:43:43.72 +06:55:30.5
02:57:55.29 +08:10:18.8
02:59:59.96 +07:06:07.6
02:56:37.16 +01:45:05.7
02:57:00.74 +05:31:44.8
02:57:54.12 +07:26:05.2
02:56:18.34 +09:18:07.9
03:01:24.55 +07:10:56.7
02:57:29.66 +02:53:42.5
02:57:22.15 +05:20:42.6
02:55:57.77 +04:06:13.8
02:59:10.44 +08:56:21.6
02:55:25.57 +06:20:17.5
03:03:53.64 +09:45:11.1
02:56:14.93 +09:21:05.1
03:32:32.81 +07:25:31.8
03:43:28.67 +07:10:58.8
03:00:06.39 +06:38:44.5
03:49:27.30 +06:04:41.1
02:54:56.68 +01:38:57.8
03:00:12.62 +02:02:10.0
03:02:33.29 +02:04:40.8
03:03:32.99 +08:44:02.0
02:59:27.39 +06:31:39.1
02:59:30.72 +01:43:01.3
03:08:54.76 +09:51:45.2
02:59:16.27 +01:38:11.8
03:13:33.62 +07:37:43.3
03:00:36.42 +02:50:13.1
03:07:08.61 +01:29:33.2
02:56:45.33 +05:17:06.0
02:56:19.85 +03:40:48.2
03:36:19.38 +04:35:45.8
02:58:42.40 +05:34:33.7
03:01:43.48 +09:24:11.1
02:59:43.92 +08:44:48.3
03:09:08.33 +10:57:07.6
03:09:53.66 +10:01:58.2
03:03:06.80 +02:01:27.9
03:01:46.89 +09:56:00.0
02:58:55.18 +03:00:13.0
02:58:01.54 +03:47:53.2
03:05:24.21 +08:21:19.0
02:58:51.62 +05:04:53.6
03:00:02.07 +02:56:08.1
03:03:54.16 +05:14:27.1
03:03:51.10 +03:51:53.7
02:58:13.23 +04:21:34.0
03:03:34.41 +07:25:33.1
03:04:00.64 +09:39:57.9
03:00:20.03 +01:24:56.7
02:57:54.79 +08:10:19.7
03:02:41.61 +07:04:00.7
03:01:26.74 +02:07:53.8
03:02:10.03 +07:51:21.4
02:58:13.45 +03:10:02.9
03:01:45.83 +07:16:41.8
02:57:10.21 +08:34:18.4
03:09:22.26 +10:48:44.2
02:57:44.32 +06:54:45.2
02:56:14.59 +03:29:04.4
03:08:49.16 +10:59:45.0
03:00:26.59 +02:10:54.9
02:55:44.79 +04:39:46.4
03:04:50.92 +08:23:38.9
02:54:33.08 +02:36:46.1
03:01:50.71 +07:44:29.8
03:00:38.54 +02:34:32.9
03:07:24.85 +10:40:47.5
02:55:58.76 +06:07:28.3
03:05:38.22 +10:39:28.4
02:59:40.18 +02:17:19.5
02:58:59.80 +07:18:50.7
02:59:21.12 +01:44:14.1
03:03:23.85 +08:38:29.7
02:58:04.98 +07:34:12.7
02:59:09.94 +08:56:18.7
02:56:33.58 +03:47:53.5
02:59:41.13 +04:05:57.7
02:56:14.34 +03:34:42.2
02:56:42.32 +06:42:12.7
02:58:00.37 +10:14:03.0
03:02:25.30 +08:25:00.4
03:01:46.00 +09:26:34.2
03:01:54.94 +08:42:56.5
03:01:12.43 +03:59:49.7
02:57:38.17 +07:10:43.2
02:59:57.50 +07:58:29.0
03:00:03.90 +06:07:39.1
02:56:19.99 +04:20:15.9
03:01:53.16 +08:37:34.2
02:56:15.97 +05:56:08.4
03:07:00.94 +09:59:55.2
02:54:43.18 +06:06:52.2
02:59:38.01 +04:18:36.6
03:01:09.19 +08:51:04.5
03:01:49.27 +01:45:00.7
02:56:58.22 +10:28:48.8
03:01:26.91 +07:51:39.4
02:56:03.69 +08:45:06.3
03:01:39.22 +10:56:36.6
03:05:58.16 +10:47:15.0
02:57:41.86 +06:06:30.2
02:55:52.85 +08:44:58.6
03:04:02.95 +08:52:23.5
02:59:30.77 +01:53:09.5
02:57:20.36 +06:40:58.5
02:59:45.17 +06:40:31.3
03:03:44.89 +01:33:56.2
02:55:40.66 +02:21:05.1
03:00:01.93 +08:56:49.8
02:56:10.90 +07:26:34.0
03:00:31.18 +04:10:20.8
02:55:34.96 +07:10:30.4
02:59:29.84 +08:36:25.3
03:02:27.39 +09:06:15.2
02:55:43.04 +07:58:50.5
03:07:12.67 +09:25:38.9
02:59:21.95 +08:05:36.2
02:59:19.19 +06:43:39.9
03:00:07.89 +06:29:11.5
03:05:03.95 +10:43:52.5
02:56:10.86 +06:36:37.9
03:03:41.88 +01:49:42.3
03:07:14.37 +10:04:46.6
03:08:03.60 +10:31:03.5
03:01:09.60 +09:34:27.2
03:00:38.56 +04:56:32.1
03:00:19.03 +06:55:50.4
02:54:32.60 +02:37:24.8
02:59:02.74 +01:43:49.5
02:58:59.92 +02:05:21.1
03:00:04.63 +08:01:20.3
03:04:17.92 +01:53:40.7
02:55:42.07 +06:33:54.6
03:07:04.56 +09:22:49.6
03:08:39.46 +10:21:21.9
02:56:34.92 +06:52:25.2
02:55:10.45 +06:45:30.3
02:54:59.90 +07:10:06.7
02:57:35.03 +06:25:56.7
02:55:53.94 +07:56:29.2
03:10:06.73 +10:49:44.3
02:58:06.51 +04:15:45.8
03:08:13.12 +10:27:57.6
02:58:01.01 +04:03:51.3
02:56:00.58 +08:20:54.8
02:57:25.76 +09:21:31.7
03:04:18.42 +10:06:38.1
02:56:46.07 +06:35:13.1
02:57:29.05 +09:10:22.3
03:03:33.42 +10:28:16.0
02:57:41.71 +09:19:29.7
02:57:11.55 +05:55:21.5
02:56:40.72 +06:31:51.8
03:01:56.46 +09:21:13.9
02:55:51.25 +09:28:24.6
02:59:32.12 +08:46:25.1
02:56:43.82 +07:32:34.6
02:54:51.53 +03:14:11.0
02:57:42.56 +05:07:42.3
02:56:39.12 +07:45:02.0
03:00:08.88 +09:09:17.4
02:58:50.41 +11:04:11.0
02:59:50.18 +08:39:15.4
02:58:43.18 +07:30:54.9
02:57:21.53 +08:31:15.9
02:57:28.61 +09:30:30.4
02:55:12.60 +07:58:16.3
02:56:21.38 +05:03:29.6
02:56:55.98 +07:27:40.5
02:57:31.75 +09:43:00.6
02:58:45.92 +05:34:00.3
03:54:42.71 +03:48:09.1
02:59:49.76 +08:39:22.7
02:56:45.63 +08:58:09.7
02:58:43.82 +07:30:56.8
02:56:23.14 +10:02:52.0
02:55:57.36 +05:48:24.1
02:57:21.79 +08:31:16.9
03:01:37.89 +01:39:16.5
03:06:37.50 +08:33:57.7
02:56:29.06 +08:15:07.9
03:00:26.32 +09:32:43.1
02:55:32.55 +05:39:00.1
02:55:00.02 +05:08:34.7
02:58:33.50 +06:32:57.8
02:59:54.00 +09:33:22.5
02:57:00.98 +10:18:57.8
02:56:46.27 +08:58:16.0
02:56:16.75 +02:23:25.3
02:57:44.59 +04:12:40.7
02:57:09.71 +09:07:06.7
02:56:28.13 +07:58:26.8
02:57:52.14 +08:54:55.3
02:56:32.99 +03:38:58.6
02:59:21.49 +08:29:43.5
02:55:12.29 +03:58:25.6
02:54:58.43 +06:39:42.5
02:56:17.09 +08:50:58.7
02:56:12.42 +03:11:47.8
02:56:38.19 +04:11:58.9
02:59:10.30 +10:42:38.3
02:55:34.42 +03:04:54.8
02:55:47.39 +04:23:25.6
03:00:13.07 +02:29:49.2
03:00:08.75 +02:26:30.9
03:00:49.95 +02:07:34.3
02:55:46.62 +09:23:51.4
02:56:19.18 +05:05:07.9
02:59:14.85 +09:24:35.1
02:56:33.61 +03:38:56.3
03:00:29.52 +04:51:26.8
02:56:54.35 +09:32:25.2
02:55:13.22 +04:01:40.8
02:56:00.70 +02:31:46.5
03:00:57.43 +09:20:44.8
02:57:24.89 +02:11:05.3
02:54:36.69 +03:25:36.5
02:56:12.32 +09:28:07.5
02:58:08.35 +08:29:43.4
02:56:51.75 +07:49:26.7
02:58:31.58 +07:00:19.1
02:55:57.49 +01:47:16.8
02:59:14.88 +05:43:36.0
########### Completed Tau-07-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 ####
03:03:15.85 +02:54:13.0
03:08:49.45 +10:59:39.3
03:05:03.70 +01:54:25.8
03:01:59.53 +03:47:58.8
03:08:30.43 +10:26:48.3
03:02:29.86 +05:35:05.8
03:03:01.41 +03:55:34.9
02:55:44.35 +07:16:52.7
02:55:31.51 +06:18:23.6
02:59:29.95 +06:20:18.8
02:55:17.13 +08:08:18.0
03:00:34.21 +10:48:04.6
02:58:12.40 +03:49:34.6
02:56:21.01 +06:33:59.0
03:03:06.96 +10:06:04.1
02:55:27.55 +06:57:40.4
03:43:43.72 +06:55:30.5
02:57:55.29 +08:10:18.8
02:59:59.96 +07:06:07.6
02:56:37.16 +01:45:05.7
02:57:00.74 +05:31:44.8
02:57:54.12 +07:26:05.2
02:56:18.34 +09:18:07.9
03:01:24.55 +07:10:56.7
02:57:29.66 +02:53:42.5
02:57:22.15 +05:20:42.6
02:55:57.77 +04:06:13.8
02:59:10.44 +08:56:21.6
02:55:25.57 +06:20:17.5
03:03:53.64 +09:45:11.1
02:56:14.93 +09:21:05.1
03:29:25.82 +06:19:09.0
03:23:43.97 +03:53:23.5
03:23:35.75 +09:23:52.0
03:00:12.62 +02:02:10.0
03:02:33.29 +02:04:40.8
03:03:32.99 +08:44:02.0
02:59:27.39 +06:31:39.1
02:59:30.72 +01:43:01.3
03:08:54.76 +09:51:45.2
02:59:16.27 +01:38:11.8
03:13:33.62 +07:37:43.3
03:00:36.42 +02:50:13.1
03:07:08.61 +01:29:33.2
02:56:45.33 +05:17:06.0
02:56:19.85 +03:40:48.2
03:36:19.38 +04:35:45.8
02:58:42.40 +05:34:33.7
03:01:43.48 +09:24:11.1
02:59:43.92 +08:44:48.3
03:09:08.33 +10:57:07.6
03:09:53.66 +10:01:58.2
03:03:06.80 +02:01:27.9
03:01:46.89 +09:56:00.0
02:58:55.18 +03:00:13.0
02:58:01.54 +03:47:53.2
03:05:24.21 +08:21:19.0
02:58:51.62 +05:04:53.6
03:00:02.07 +02:56:08.1
03:03:54.16 +05:14:27.1
03:03:51.10 +03:51:53.7
02:58:13.23 +04:21:34.0
03:03:34.41 +07:25:33.1
03:04:00.64 +09:39:57.9
03:00:20.03 +01:24:56.7
02:57:54.79 +08:10:19.7
03:02:41.61 +07:04:00.7
03:01:26.74 +02:07:53.8
03:02:10.03 +07:51:21.4
02:58:13.45 +03:10:02.9
03:01:45.83 +07:16:41.8
02:57:10.21 +08:34:18.4
03:09:22.26 +10:48:44.2
02:57:44.32 +06:54:45.2
02:56:14.59 +03:29:04.4
03:08:49.16 +10:59:45.0
03:00:26.59 +02:10:54.9
02:55:44.79 +04:39:46.4
03:04:50.92 +08:23:38.9
02:54:33.08 +02:36:46.1
03:01:50.71 +07:44:29.8
03:00:38.54 +02:34:32.9
03:07:24.85 +10:40:47.5
02:55:58.76 +06:07:28.3
03:05:38.22 +10:39:28.4
02:59:40.18 +02:17:19.5
02:58:59.80 +07:18:50.7
02:59:21.12 +01:44:14.1
03:03:23.85 +08:38:29.7
02:58:04.98 +07:34:12.7
02:59:09.94 +08:56:18.7
02:56:33.58 +03:47:53.5
02:59:41.13 +04:05:57.7
02:56:14.34 +03:34:42.2
02:56:42.32 +06:42:12.7
02:58:00.37 +10:14:03.0
03:02:25.30 +08:25:00.4
03:01:46.00 +09:26:34.2
03:01:54.94 +08:42:56.5
03:01:12.43 +03:59:49.7
02:57:38.17 +07:10:43.2
02:59:57.50 +07:58:29.0
03:00:03.90 +06:07:39.1
02:56:19.99 +04:20:15.9
03:01:53.16 +08:37:34.2
02:56:15.97 +05:56:08.4
03:07:00.94 +09:59:55.2
02:54:43.18 +06:06:52.2
02:59:38.01 +04:18:36.6
03:01:09.19 +08:51:04.5
03:01:49.27 +01:45:00.7
02:56:58.22 +10:28:48.8
03:01:26.91 +07:51:39.4
02:56:03.69 +08:45:06.3
03:01:39.22 +10:56:36.6
03:05:58.16 +10:47:15.0
02:57:41.86 +06:06:30.2
02:55:52.85 +08:44:58.6
03:04:02.95 +08:52:23.5
02:59:30.77 +01:53:09.5
02:57:20.36 +06:40:58.5
02:59:45.17 +06:40:31.3
03:03:44.89 +01:33:56.2
02:55:40.66 +02:21:05.1
03:00:01.93 +08:56:49.8
02:56:10.90 +07:26:34.0
03:00:31.18 +04:10:20.8
02:55:34.96 +07:10:30.4
02:59:29.84 +08:36:25.3
03:02:27.39 +09:06:15.2
02:55:43.04 +07:58:50.5
03:07:12.67 +09:25:38.9
02:59:21.95 +08:05:36.2
02:59:19.19 +06:43:39.9
03:00:07.89 +06:29:11.5
03:05:03.95 +10:43:52.5
02:56:10.86 +06:36:37.9
03:03:41.88 +01:49:42.3
03:07:14.37 +10:04:46.6
03:08:03.60 +10:31:03.5
03:01:09.60 +09:34:27.2
03:00:38.56 +04:56:32.1
03:00:19.03 +06:55:50.4
02:54:32.60 +02:37:24.8
02:59:02.74 +01:43:49.5
02:58:59.92 +02:05:21.1
03:00:04.63 +08:01:20.3
03:04:17.92 +01:53:40.7
02:55:42.07 +06:33:54.6
03:07:04.56 +09:22:49.6
03:08:39.46 +10:21:21.9
02:56:34.92 +06:52:25.2
02:55:10.45 +06:45:30.3
02:54:59.90 +07:10:06.7
02:57:35.03 +06:25:56.7
02:55:53.94 +07:56:29.2
03:10:06.73 +10:49:44.3
02:58:06.51 +04:15:45.8
03:08:13.12 +10:27:57.6
02:58:01.01 +04:03:51.3
02:56:00.58 +08:20:54.8
02:57:25.76 +09:21:31.7
03:04:18.42 +10:06:38.1
02:56:46.07 +06:35:13.1
02:57:29.05 +09:10:22.3
03:03:33.42 +10:28:16.0
02:57:41.71 +09:19:29.7
02:57:11.55 +05:55:21.5
02:56:40.72 +06:31:51.8
03:01:56.46 +09:21:13.9
02:55:51.25 +09:28:24.6
02:59:32.12 +08:46:25.1
02:56:43.82 +07:32:34.6
02:54:51.53 +03:14:11.0
02:57:42.56 +05:07:42.3
02:56:39.12 +07:45:02.0
03:00:08.88 +09:09:17.4
02:58:50.41 +11:04:11.0
02:59:50.18 +08:39:15.4
02:58:43.18 +07:30:54.9
02:57:21.53 +08:31:15.9
02:57:28.61 +09:30:30.4
02:55:12.60 +07:58:16.3
02:56:21.38 +05:03:29.6
02:56:55.98 +07:27:40.5
02:57:31.75 +09:43:00.6
02:58:45.92 +05:34:00.3
03:54:42.71 +03:48:09.1
02:59:49.76 +08:39:22.7
02:56:45.63 +08:58:09.7
02:58:43.82 +07:30:56.8
02:56:23.14 +10:02:52.0
02:55:57.36 +05:48:24.1
02:57:21.79 +08:31:16.9
03:01:37.89 +01:39:16.5
03:06:37.50 +08:33:57.7
02:56:29.06 +08:15:07.9
03:00:26.32 +09:32:43.1
02:55:32.55 +05:39:00.1
02:55:00.02 +05:08:34.7
02:58:33.50 +06:32:57.8
02:59:54.00 +09:33:22.5
02:57:00.98 +10:18:57.8
02:56:46.27 +08:58:16.0
02:56:16.75 +02:23:25.3
02:57:44.59 +04:12:40.7
02:57:09.71 +09:07:06.7
02:56:28.13 +07:58:26.8
02:57:52.14 +08:54:55.3
02:56:32.99 +03:38:58.6
02:59:21.49 +08:29:43.5
02:55:12.29 +03:58:25.6
02:54:58.43 +06:39:42.5
02:56:17.09 +08:50:58.7
02:56:12.42 +03:11:47.8
02:56:38.19 +04:11:58.9
02:59:10.30 +10:42:38.3
02:55:34.42 +03:04:54.8
02:55:47.39 +04:23:25.6
03:00:13.07 +02:29:49.2
03:00:08.75 +02:26:30.9
03:00:49.95 +02:07:34.3
02:55:46.62 +09:23:51.4
02:56:19.18 +05:05:07.9
02:59:14.85 +09:24:35.1
02:56:33.61 +03:38:56.3
03:00:29.52 +04:51:26.8
02:56:54.35 +09:32:25.2
02:55:13.22 +04:01:40.8
02:56:00.70 +02:31:46.5
03:00:57.43 +09:20:44.8
02:57:24.89 +02:11:05.3
02:54:36.69 +03:25:36.5
02:56:12.32 +09:28:07.5
02:58:08.35 +08:29:43.4
02:56:51.75 +07:49:26.7
02:58:31.58 +07:00:19.1
02:55:57.49 +01:47:16.8
02:59:14.88 +05:43:36.0
03:32:32.81 +07:25:31.8
03:49:27.30 +06:04:41.1
02:54:56.68 +01:38:57.8
03:43:28.67 +07:10:58.8
03:00:06.39 +06:38:44.5
###################################################################################
03:03:15.85 +02:54:13.0 -- not an asteroid (will add it to exclusion list)
03:08:49.45 +10:59:39.3 -- not an asteroid (will add it to exclusion list)
03:05:03.70 +01:54:25.8 -- not an asteroid (will add it to exclusion list)
03:01:59.53 +03:47:58.8 -- not an asteroid (will add it to exclusion list)
03:08:30.43 +10:26:48.3 -- not an asteroid (will add it to exclusion list)
03:02:29.86 +05:35:05.8 -- not an asteroid (will add it to exclusion list)
03:03:01.41 +03:55:34.9 -- not an asteroid (will add it to exclusion list)
02:55:44.35 +07:16:52.7 -- not an asteroid (will add it to exclusion list)
02:55:31.51 +06:18:23.6 -- not an asteroid (will add it to exclusion list)
02:59:29.95 +06:20:18.8 -- not an asteroid (will add it to exclusion list)
02:55:17.13 +08:08:18.0 -- not an asteroid (will add it to exclusion list)
03:00:34.21 +10:48:04.6 -- not an asteroid (will add it to exclusion list)
02:58:12.40 +03:49:34.6 -- not an asteroid (will add it to exclusion list)
02:56:21.01 +06:33:59.0 -- not an asteroid (will add it to exclusion list)
03:03:06.96 +10:06:04.1 -- not an asteroid (will add it to exclusion list)
02:55:27.55 +06:57:40.4 -- not an asteroid (will add it to exclusion list)
03:43:43.72 +06:55:30.5 -- not an asteroid (will add it to exclusion list)
02:57:55.29 +08:10:18.8 -- not an asteroid (will add it to exclusion list)
02:59:59.96 +07:06:07.6 -- not an asteroid (will add it to exclusion list)
02:56:37.16 +01:45:05.7 -- not an asteroid (will add it to exclusion list)
02:57:00.74 +05:31:44.8 -- not an asteroid (will add it to exclusion list)
02:57:54.12 +07:26:05.2 -- not an asteroid (will add it to exclusion list)
02:56:18.34 +09:18:07.9 -- not an asteroid (will add it to exclusion list)
03:01:24.55 +07:10:56.7 -- not an asteroid (will add it to exclusion list)
02:57:29.66 +02:53:42.5 -- not an asteroid (will add it to exclusion list)
02:57:22.15 +05:20:42.6 -- not an asteroid (will add it to exclusion list)
02:55:57.77 +04:06:13.8 -- not an asteroid (will add it to exclusion list)
02:59:10.44 +08:56:21.6 -- not an asteroid (will add it to exclusion list)
02:55:25.57 +06:20:17.5 -- not an asteroid (will add it to exclusion list)
03:03:53.64 +09:45:11.1 -- not an asteroid (will add it to exclusion list)
02:56:14.93 +09:21:05.1 -- not an asteroid (will add it to exclusion list)
03:29:25.82 +06:19:09.0 -- not an asteroid (will add it to exclusion list)
03:23:43.97 +03:53:23.5 -- not an asteroid (will add it to exclusion list)
03:23:35.75 +09:23:52.0 -- not an asteroid (will add it to exclusion list)
03:00:12.62 +02:02:10.0 -- not an asteroid (will add it to exclusion list)
03:02:33.29 +02:04:40.8 -- not an asteroid (will add it to exclusion list)
03:03:32.99 +08:44:02.0 -- not an asteroid (will add it to exclusion list)
02:59:27.39 +06:31:39.1 -- not an asteroid (will add it to exclusion list)
02:59:30.72 +01:43:01.3 -- not an asteroid (will add it to exclusion list)
03:08:54.76 +09:51:45.2 -- not an asteroid (will add it to exclusion list)
02:59:16.27 +01:38:11.8 -- not an asteroid (will add it to exclusion list)
03:13:33.62 +07:37:43.3 -- not an asteroid (will add it to exclusion list)
03:00:36.42 +02:50:13.1 -- not an asteroid (will add it to exclusion list)
03:07:08.61 +01:29:33.2 -- not an asteroid (will add it to exclusion list)
02:56:45.33 +05:17:06.0 -- not an asteroid (will add it to exclusion list)
02:56:19.85 +03:40:48.2 -- not an asteroid (will add it to exclusion list)
03:36:19.38 +04:35:45.8 -- not an asteroid (will add it to exclusion list)
02:58:42.40 +05:34:33.7 -- not an asteroid (will add it to exclusion list)
03:01:43.48 +09:24:11.1 -- not an asteroid (will add it to exclusion list)
02:59:43.92 +08:44:48.3 -- not an asteroid (will add it to exclusion list)
03:09:08.33 +10:57:07.6 -- not an asteroid (will add it to exclusion list)
03:09:53.66 +10:01:58.2 -- not an asteroid (will add it to exclusion list)
03:03:06.80 +02:01:27.9 -- not an asteroid (will add it to exclusion list)
03:01:46.89 +09:56:00.0 -- not an asteroid (will add it to exclusion list)
02:58:55.18 +03:00:13.0 -- not an asteroid (will add it to exclusion list)
02:58:01.54 +03:47:53.2 -- not an asteroid (will add it to exclusion list)
03:05:24.21 +08:21:19.0 -- not an asteroid (will add it to exclusion list)
02:58:51.62 +05:04:53.6 -- not an asteroid (will add it to exclusion list)
03:00:02.07 +02:56:08.1 -- not an asteroid (will add it to exclusion list)
03:03:54.16 +05:14:27.1 -- not an asteroid (will add it to exclusion list)
03:03:51.10 +03:51:53.7 -- not an asteroid (will add it to exclusion list)
02:58:13.23 +04:21:34.0 -- not an asteroid (will add it to exclusion list)
03:03:34.41 +07:25:33.1 -- not an asteroid (will add it to exclusion list)
03:04:00.64 +09:39:57.9 -- not an asteroid (will add it to exclusion list)
03:00:20.03 +01:24:56.7 -- not an asteroid (will add it to exclusion list)
02:57:54.79 +08:10:19.7 -- not an asteroid (will add it to exclusion list)
03:02:41.61 +07:04:00.7 -- not an asteroid (will add it to exclusion list)
03:01:26.74 +02:07:53.8 -- not an asteroid (will add it to exclusion list)
03:02:10.03 +07:51:21.4 -- not an asteroid (will add it to exclusion list)
02:58:13.45 +03:10:02.9 -- not an asteroid (will add it to exclusion list)
03:01:45.83 +07:16:41.8 -- not an asteroid (will add it to exclusion list)
02:57:10.21 +08:34:18.4 -- not an asteroid (will add it to exclusion list)
03:09:22.26 +10:48:44.2 -- not an asteroid (will add it to exclusion list)
02:57:44.32 +06:54:45.2 -- not an asteroid (will add it to exclusion list)
02:56:14.59 +03:29:04.4 -- not an asteroid (will add it to exclusion list)
03:08:49.16 +10:59:45.0 -- not an asteroid (will add it to exclusion list)
03:00:26.59 +02:10:54.9 -- not an asteroid (will add it to exclusion list)
02:55:44.79 +04:39:46.4 -- not an asteroid (will add it to exclusion list)
03:04:50.92 +08:23:38.9 -- not an asteroid (will add it to exclusion list)
02:54:33.08 +02:36:46.1 -- not an asteroid (will add it to exclusion list)
03:01:50.71 +07:44:29.8 -- not an asteroid (will add it to exclusion list)
03:00:38.54 +02:34:32.9 -- not an asteroid (will add it to exclusion list)
03:07:24.85 +10:40:47.5 -- not an asteroid (will add it to exclusion list)
02:55:58.76 +06:07:28.3 -- not an asteroid (will add it to exclusion list)
03:05:38.22 +10:39:28.4 -- not an asteroid (will add it to exclusion list)
02:59:40.18 +02:17:19.5 -- not an asteroid (will add it to exclusion list)
02:58:59.80 +07:18:50.7 -- not an asteroid (will add it to exclusion list)
02:59:21.12 +01:44:14.1 -- not an asteroid (will add it to exclusion list)
03:03:23.85 +08:38:29.7 -- not an asteroid (will add it to exclusion list)
02:58:04.98 +07:34:12.7 -- not an asteroid (will add it to exclusion list)
02:59:09.94 +08:56:18.7 -- not an asteroid (will add it to exclusion list)
02:56:33.58 +03:47:53.5 -- not an asteroid (will add it to exclusion list)
02:59:41.13 +04:05:57.7 -- not an asteroid (will add it to exclusion list)
02:56:14.34 +03:34:42.2 -- not an asteroid (will add it to exclusion list)
02:56:42.32 +06:42:12.7 -- not an asteroid (will add it to exclusion list)
02:58:00.37 +10:14:03.0 -- not an asteroid (will add it to exclusion list)
03:02:25.30 +08:25:00.4 -- asteroid (will NOT add it to exclusion list)
03:01:46.00 +09:26:34.2 -- not an asteroid (will add it to exclusion list)
03:01:54.94 +08:42:56.5 -- not an asteroid (will add it to exclusion list)
03:01:12.43 +03:59:49.7 -- not an asteroid (will add it to exclusion list)
02:57:38.17 +07:10:43.2 -- not an asteroid (will add it to exclusion list)
02:59:57.50 +07:58:29.0 -- not an asteroid (will add it to exclusion list)
03:00:03.90 +06:07:39.1 -- not an asteroid (will add it to exclusion list)
02:56:19.99 +04:20:15.9 -- not an asteroid (will add it to exclusion list)
03:01:53.16 +08:37:34.2 -- not an asteroid (will add it to exclusion list)
02:56:15.97 +05:56:08.4 -- not an asteroid (will add it to exclusion list)
03:07:00.94 +09:59:55.2 -- not an asteroid (will add it to exclusion list)
02:54:43.18 +06:06:52.2 -- not an asteroid (will add it to exclusion list)
02:59:38.01 +04:18:36.6 -- not an asteroid (will add it to exclusion list)
03:01:09.19 +08:51:04.5 -- not an asteroid (will add it to exclusion list)
03:01:49.27 +01:45:00.7 -- not an asteroid (will add it to exclusion list)
02:56:58.22 +10:28:48.8 -- not an asteroid (will add it to exclusion list)
03:01:26.91 +07:51:39.4 -- not an asteroid (will add it to exclusion list)
02:56:03.69 +08:45:06.3 -- not an asteroid (will add it to exclusion list)
03:01:39.22 +10:56:36.6 -- not an asteroid (will add it to exclusion list)
03:05:58.16 +10:47:15.0 -- not an asteroid (will add it to exclusion list)
02:57:41.86 +06:06:30.2 -- not an asteroid (will add it to exclusion list)
02:55:52.85 +08:44:58.6 -- not an asteroid (will add it to exclusion list)
03:04:02.95 +08:52:23.5 -- not an asteroid (will add it to exclusion list)
02:59:30.77 +01:53:09.5 -- not an asteroid (will add it to exclusion list)
02:57:20.36 +06:40:58.5 -- not an asteroid (will add it to exclusion list)
02:59:45.17 +06:40:31.3 -- not an asteroid (will add it to exclusion list)
03:03:44.89 +01:33:56.2 -- not an asteroid (will add it to exclusion list)
02:55:40.66 +02:21:05.1 -- not an asteroid (will add it to exclusion list)
03:00:01.93 +08:56:49.8 -- not an asteroid (will add it to exclusion list)
02:56:10.90 +07:26:34.0 -- not an asteroid (will add it to exclusion list)
03:00:31.18 +04:10:20.8 -- not an asteroid (will add it to exclusion list)
02:55:34.96 +07:10:30.4 -- not an asteroid (will add it to exclusion list)
02:59:29.84 +08:36:25.3 -- not an asteroid (will add it to exclusion list)
03:02:27.39 +09:06:15.2 -- not an asteroid (will add it to exclusion list)
02:55:43.04 +07:58:50.5 -- not an asteroid (will add it to exclusion list)
03:07:12.67 +09:25:38.9 -- not an asteroid (will add it to exclusion list)
02:59:21.95 +08:05:36.2 -- not an asteroid (will add it to exclusion list)
02:59:19.19 +06:43:39.9 -- not an asteroid (will add it to exclusion list)
03:00:07.89 +06:29:11.5 -- not an asteroid (will add it to exclusion list)
03:05:03.95 +10:43:52.5 -- not an asteroid (will add it to exclusion list)
02:56:10.86 +06:36:37.9 -- not an asteroid (will add it to exclusion list)
03:03:41.88 +01:49:42.3 -- not an asteroid (will add it to exclusion list)
03:07:14.37 +10:04:46.6 -- not an asteroid (will add it to exclusion list)
03:08:03.60 +10:31:03.5 -- not an asteroid (will add it to exclusion list)
03:01:09.60 +09:34:27.2 -- not an asteroid (will add it to exclusion list)
03:00:38.56 +04:56:32.1 -- not an asteroid (will add it to exclusion list)
03:00:19.03 +06:55:50.4 -- not an asteroid (will add it to exclusion list)
02:54:32.60 +02:37:24.8 -- not an asteroid (will add it to exclusion list)
02:59:02.74 +01:43:49.5 -- not an asteroid (will add it to exclusion list)
02:58:59.92 +02:05:21.1 -- not an asteroid (will add it to exclusion list)
03:00:04.63 +08:01:20.3 -- not an asteroid (will add it to exclusion list)
03:04:17.92 +01:53:40.7 -- not an asteroid (will add it to exclusion list)
02:55:42.07 +06:33:54.6 -- not an asteroid (will add it to exclusion list)
03:07:04.56 +09:22:49.6 -- not an asteroid (will add it to exclusion list)
03:08:39.46 +10:21:21.9 -- not an asteroid (will add it to exclusion list)
02:56:34.92 +06:52:25.2 -- not an asteroid (will add it to exclusion list)
02:55:10.45 +06:45:30.3 -- not an asteroid (will add it to exclusion list)
02:54:59.90 +07:10:06.7 -- not an asteroid (will add it to exclusion list)
02:57:35.03 +06:25:56.7 -- not an asteroid (will add it to exclusion list)
02:55:53.94 +07:56:29.2 -- not an asteroid (will add it to exclusion list)
03:10:06.73 +10:49:44.3 -- not an asteroid (will add it to exclusion list)
02:58:06.51 +04:15:45.8 -- not an asteroid (will add it to exclusion list)
03:08:13.12 +10:27:57.6 -- not an asteroid (will add it to exclusion list)
02:58:01.01 +04:03:51.3 -- not an asteroid (will add it to exclusion list)
02:56:00.58 +08:20:54.8 -- not an asteroid (will add it to exclusion list)
02:57:25.76 +09:21:31.7 -- not an asteroid (will add it to exclusion list)
03:04:18.42 +10:06:38.1 -- not an asteroid (will add it to exclusion list)
02:56:46.07 +06:35:13.1 -- not an asteroid (will add it to exclusion list)
02:57:29.05 +09:10:22.3 -- not an asteroid (will add it to exclusion list)
03:03:33.42 +10:28:16.0 -- not an asteroid (will add it to exclusion list)
02:57:41.71 +09:19:29.7 -- not an asteroid (will add it to exclusion list)
02:57:11.55 +05:55:21.5 -- not an asteroid (will add it to exclusion list)
02:56:40.72 +06:31:51.8 -- not an asteroid (will add it to exclusion list)
03:01:56.46 +09:21:13.9 -- not an asteroid (will add it to exclusion list)
02:55:51.25 +09:28:24.6 -- not an asteroid (will add it to exclusion list)
02:59:32.12 +08:46:25.1 -- not an asteroid (will add it to exclusion list)
02:56:43.82 +07:32:34.6 -- not an asteroid (will add it to exclusion list)
02:54:51.53 +03:14:11.0 -- not an asteroid (will add it to exclusion list)
02:57:42.56 +05:07:42.3 -- not an asteroid (will add it to exclusion list)
02:56:39.12 +07:45:02.0 -- not an asteroid (will add it to exclusion list)
03:00:08.88 +09:09:17.4 -- not an asteroid (will add it to exclusion list)
02:58:50.41 +11:04:11.0 -- not an asteroid (will add it to exclusion list)
02:59:50.18 +08:39:15.4 -- not an asteroid (will add it to exclusion list)
02:58:43.18 +07:30:54.9 -- not an asteroid (will add it to exclusion list)
02:57:21.53 +08:31:15.9 -- not an asteroid (will add it to exclusion list)
02:57:28.61 +09:30:30.4 -- not an asteroid (will add it to exclusion list)
02:55:12.60 +07:58:16.3 -- not an asteroid (will add it to exclusion list)
02:56:21.38 +05:03:29.6 -- not an asteroid (will add it to exclusion list)
02:56:55.98 +07:27:40.5 -- not an asteroid (will add it to exclusion list)
02:57:31.75 +09:43:00.6 -- not an asteroid (will add it to exclusion list)
02:58:45.92 +05:34:00.3 -- not an asteroid (will add it to exclusion list)
03:54:42.71 +03:48:09.1 -- asteroid (will NOT add it to exclusion list)
02:59:49.76 +08:39:22.7 -- not an asteroid (will add it to exclusion list)
02:56:45.63 +08:58:09.7 -- not an asteroid (will add it to exclusion list)
02:58:43.82 +07:30:56.8 -- not an asteroid (will add it to exclusion list)
02:56:23.14 +10:02:52.0 -- not an asteroid (will add it to exclusion list)
02:55:57.36 +05:48:24.1 -- not an asteroid (will add it to exclusion list)
02:57:21.79 +08:31:16.9 -- not an asteroid (will add it to exclusion list)
03:01:37.89 +01:39:16.5 -- not an asteroid (will add it to exclusion list)
03:06:37.50 +08:33:57.7 -- not an asteroid (will add it to exclusion list)
02:56:29.06 +08:15:07.9 -- not an asteroid (will add it to exclusion list)
03:00:26.32 +09:32:43.1 -- not an asteroid (will add it to exclusion list)
02:55:32.55 +05:39:00.1 -- not an asteroid (will add it to exclusion list)
02:55:00.02 +05:08:34.7 -- not an asteroid (will add it to exclusion list)
02:58:33.50 +06:32:57.8 -- not an asteroid (will add it to exclusion list)
02:59:54.00 +09:33:22.5 -- not an asteroid (will add it to exclusion list)
02:57:00.98 +10:18:57.8 -- not an asteroid (will add it to exclusion list)
02:56:46.27 +08:58:16.0 -- not an asteroid (will add it to exclusion list)
02:56:16.75 +02:23:25.3 -- not an asteroid (will add it to exclusion list)
02:57:44.59 +04:12:40.7 -- not an asteroid (will add it to exclusion list)
02:57:09.71 +09:07:06.7 -- not an asteroid (will add it to exclusion list)
02:56:28.13 +07:58:26.8 -- not an asteroid (will add it to exclusion list)
02:57:52.14 +08:54:55.3 -- not an asteroid (will add it to exclusion list)
02:56:32.99 +03:38:58.6 -- not an asteroid (will add it to exclusion list)
02:59:21.49 +08:29:43.5 -- not an asteroid (will add it to exclusion list)
02:55:12.29 +03:58:25.6 -- not an asteroid (will add it to exclusion list)
02:54:58.43 +06:39:42.5 -- not an asteroid (will add it to exclusion list)
02:56:17.09 +08:50:58.7 -- not an asteroid (will add it to exclusion list)
02:56:12.42 +03:11:47.8 -- not an asteroid (will add it to exclusion list)
02:56:38.19 +04:11:58.9 -- not an asteroid (will add it to exclusion list)
02:59:10.30 +10:42:38.3 -- not an asteroid (will add it to exclusion list)
02:55:34.42 +03:04:54.8 -- not an asteroid (will add it to exclusion list)
02:55:47.39 +04:23:25.6 -- not an asteroid (will add it to exclusion list)
03:00:13.07 +02:29:49.2 -- not an asteroid (will add it to exclusion list)
03:00:08.75 +02:26:30.9 -- not an asteroid (will add it to exclusion list)
03:00:49.95 +02:07:34.3 -- not an asteroid (will add it to exclusion list)
02:55:46.62 +09:23:51.4 -- not an asteroid (will add it to exclusion list)
02:56:19.18 +05:05:07.9 -- not an asteroid (will add it to exclusion list)
02:59:14.85 +09:24:35.1 -- not an asteroid (will add it to exclusion list)
02:56:33.61 +03:38:56.3 -- not an asteroid (will add it to exclusion list)
03:00:29.52 +04:51:26.8 -- not an asteroid (will add it to exclusion list)
02:56:54.35 +09:32:25.2 -- not an asteroid (will add it to exclusion list)
02:55:13.22 +04:01:40.8 -- not an asteroid (will add it to exclusion list)
02:56:00.70 +02:31:46.5 -- not an asteroid (will add it to exclusion list)
03:00:57.43 +09:20:44.8 -- not an asteroid (will add it to exclusion list)
02:57:24.89 +02:11:05.3 -- not an asteroid (will add it to exclusion list)
02:54:36.69 +03:25:36.5 -- not an asteroid (will add it to exclusion list)
02:56:12.32 +09:28:07.5 -- not an asteroid (will add it to exclusion list)
02:58:08.35 +08:29:43.4 -- not an asteroid (will add it to exclusion list)
02:56:51.75 +07:49:26.7 -- not an asteroid (will add it to exclusion list)
02:58:31.58 +07:00:19.1 -- not an asteroid (will add it to exclusion list)
02:55:57.49 +01:47:16.8 -- not an asteroid (will add it to exclusion list)
02:59:14.88 +05:43:36.0 -- not an asteroid (will add it to exclusion list)
03:32:32.81 +07:25:31.8 -- not an asteroid (will add it to exclusion list)
03:49:27.30 +06:04:41.1 -- not an asteroid (will add it to exclusion list)
02:54:56.68 +01:38:57.8 -- not an asteroid (will add it to exclusion list)
03:43:28.67 +07:10:58.8 -- not an asteroid (will add it to exclusion list)
03:00:06.39 +06:38:44.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
02:54:32.60 +02:37:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:33.08 +02:36:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:36.69 +03:25:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:43.18 +06:06:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:51.53 +03:14:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:56.68 +01:38:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:58.43 +06:39:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:54:59.90 +07:10:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:00.02 +05:08:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:10.45 +06:45:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:12.29 +03:58:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:12.60 +07:58:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:13.22 +04:01:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:17.13 +08:08:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:25.57 +06:20:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:27.55 +06:57:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:31.51 +06:18:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:32.55 +05:39:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:34.42 +03:04:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:34.96 +07:10:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:40.66 +02:21:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:42.07 +06:33:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:43.04 +07:58:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:44.35 +07:16:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:44.79 +04:39:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:46.62 +09:23:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:47.39 +04:23:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:51.25 +09:28:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:52.85 +08:44:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:53.94 +07:56:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:57.36 +05:48:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:57.49 +01:47:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:57.77 +04:06:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:55:58.76 +06:07:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:00.58 +08:20:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:00.70 +02:31:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:03.69 +08:45:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:10.86 +06:36:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:10.90 +07:26:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:12.32 +09:28:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:12.42 +03:11:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:14.34 +03:34:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:14.59 +03:29:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:14.93 +09:21:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:15.97 +05:56:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:16.75 +02:23:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:17.09 +08:50:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:18.34 +09:18:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:19.18 +05:05:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:19.85 +03:40:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:19.99 +04:20:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:21.01 +06:33:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:21.38 +05:03:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:23.14 +10:02:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:28.13 +07:58:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:29.06 +08:15:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:32.99 +03:38:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:33.58 +03:47:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:33.61 +03:38:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:34.92 +06:52:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:37.16 +01:45:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:38.19 +04:11:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:39.12 +07:45:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:40.72 +06:31:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:42.32 +06:42:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:43.82 +07:32:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:45.33 +05:17:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:45.63 +08:58:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:46.07 +06:35:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:46.27 +08:58:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:51.75 +07:49:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:54.35 +09:32:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:55.98 +07:27:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:56:58.22 +10:28:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:00.74 +05:31:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:00.98 +10:18:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:09.71 +09:07:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:10.21 +08:34:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:11.55 +05:55:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:20.36 +06:40:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:21.53 +08:31:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:21.79 +08:31:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:22.15 +05:20:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:24.89 +02:11:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:25.76 +09:21:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:28.61 +09:30:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:29.05 +09:10:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:29.66 +02:53:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:31.75 +09:43:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:35.03 +06:25:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:38.17 +07:10:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:41.71 +09:19:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:41.86 +06:06:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:42.56 +05:07:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:44.32 +06:54:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:44.59 +04:12:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:52.14 +08:54:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:54.12 +07:26:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:54.79 +08:10:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:57:55.29 +08:10:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:00.37 +10:14:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:01.01 +04:03:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:01.54 +03:47:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:04.98 +07:34:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:06.51 +04:15:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:08.35 +08:29:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:12.40 +03:49:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:13.23 +04:21:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:13.45 +03:10:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:31.58 +07:00:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:33.50 +06:32:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:42.40 +05:34:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:43.18 +07:30:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:43.82 +07:30:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:45.92 +05:34:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:50.41 +11:04:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:51.62 +05:04:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:55.18 +03:00:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:59.80 +07:18:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:58:59.92 +02:05:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:02.74 +01:43:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:09.94 +08:56:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:10.30 +10:42:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:10.44 +08:56:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:14.85 +09:24:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:14.88 +05:43:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:16.27 +01:38:11.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:19.19 +06:43:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:21.12 +01:44:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:21.49 +08:29:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:21.95 +08:05:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:27.39 +06:31:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:29.84 +08:36:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:29.95 +06:20:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:30.72 +01:43:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:30.77 +01:53:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:32.12 +08:46:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:38.01 +04:18:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:40.18 +02:17:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:41.13 +04:05:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:43.92 +08:44:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:45.17 +06:40:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:49.76 +08:39:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:50.18 +08:39:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:54.00 +09:33:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:57.50 +07:58:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
02:59:59.96 +07:06:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:01.93 +08:56:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:02.07 +02:56:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:03.90 +06:07:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:04.63 +08:01:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:06.39 +06:38:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:07.89 +06:29:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:08.75 +02:26:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:08.88 +09:09:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:12.62 +02:02:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:13.07 +02:29:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:19.03 +06:55:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:20.03 +01:24:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:26.32 +09:32:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:26.59 +02:10:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:29.52 +04:51:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:31.18 +04:10:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:34.21 +10:48:04.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:36.42 +02:50:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:38.54 +02:34:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:38.56 +04:56:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:49.95 +02:07:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:00:57.43 +09:20:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:09.19 +08:51:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:09.60 +09:34:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:12.43 +03:59:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:24.55 +07:10:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:26.74 +02:07:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:26.91 +07:51:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:37.89 +01:39:16.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:39.22 +10:56:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:43.48 +09:24:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:45.83 +07:16:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:46.00 +09:26:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:46.89 +09:56:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:49.27 +01:45:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:50.71 +07:44:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:53.16 +08:37:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:54.94 +08:42:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:56.46 +09:21:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:01:59.53 +03:47:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:02:10.03 +07:51:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:02:27.39 +09:06:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:02:29.86 +05:35:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:02:33.29 +02:04:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:02:41.61 +07:04:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:01.41 +03:55:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:06.80 +02:01:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:06.96 +10:06:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:15.85 +02:54:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:23.85 +08:38:29.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:32.99 +08:44:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:33.42 +10:28:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:34.41 +07:25:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:41.88 +01:49:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:44.89 +01:33:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:51.10 +03:51:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:53.64 +09:45:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:03:54.16 +05:14:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:00.64 +09:39:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:02.95 +08:52:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:17.92 +01:53:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:18.42 +10:06:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:04:50.92 +08:23:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:05:03.70 +01:54:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:05:03.95 +10:43:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:05:24.21 +08:21:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:05:38.22 +10:39:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:05:58.16 +10:47:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:06:37.50 +08:33:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:07:00.94 +09:59:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:07:04.56 +09:22:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:07:08.61 +01:29:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:07:12.67 +09:25:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:07:14.37 +10:04:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:07:24.85 +10:40:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:03.60 +10:31:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:13.12 +10:27:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:30.43 +10:26:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:39.46 +10:21:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:49.16 +10:59:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:49.45 +10:59:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:54.76 +09:51:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:09:08.33 +10:57:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:09:22.26 +10:48:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:09:53.66 +10:01:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:10:06.73 +10:49:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:33.62 +07:37:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:35.75 +09:23:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:23:43.97 +03:53:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:29:25.82 +06:19:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:32.81 +07:25:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:19.38 +04:35:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:28.67 +07:10:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:43.72 +06:55:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:27.30 +06:04:41.1 -- 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)
02:54:32.60 +02:37:24.8 -- not a known variable star
02:54:33.08 +02:36:46.1 -- not a known variable star
02:54:36.69 +03:25:36.5 -- not a known variable star
02:54:43.18 +06:06:52.2 -- not a known variable star
02:54:51.53 +03:14:11.0 -- not a known variable star
02:54:56.68 +01:38:57.8 -- not a known variable star
02:54:58.43 +06:39:42.5 -- not a known variable star
02:54:59.90 +07:10:06.7 -- not a known variable star
02:55:00.02 +05:08:34.7 -- not a known variable star
02:55:10.45 +06:45:30.3 -- not a known variable star
02:55:12.29 +03:58:25.6 -- a known variable star
02:55:12.60 +07:58:16.3 -- a known variable star
02:55:13.22 +04:01:40.8 -- not a known variable star
02:55:17.13 +08:08:18.0 -- not a known variable star
02:55:25.57 +06:20:17.5 -- not a known variable star
02:55:27.55 +06:57:40.4 -- not a known variable star
02:55:31.51 +06:18:23.6 -- not a known variable star
02:55:32.55 +05:39:00.1 -- not a known variable star
02:55:34.42 +03:04:54.8 -- not a known variable star
02:55:34.96 +07:10:30.4 -- not a known variable star
02:55:40.66 +02:21:05.1 -- not a known variable star
02:55:42.07 +06:33:54.6 -- not a known variable star
02:55:43.04 +07:58:50.5 -- not a known variable star
02:55:44.35 +07:16:52.7 -- not a known variable star
02:55:44.79 +04:39:46.4 -- not a known variable star
02:55:46.62 +09:23:51.4 -- not a known variable star
02:55:47.39 +04:23:25.6 -- not a known variable star
02:55:51.25 +09:28:24.6 -- not a known variable star
02:55:52.85 +08:44:58.6 -- not a known variable star
02:55:53.94 +07:56:29.2 -- not a known variable star
02:55:57.36 +05:48:24.1 -- not a known variable star
02:55:57.49 +01:47:16.8 -- not a known variable star
02:55:57.77 +04:06:13.8 -- not a known variable star
02:55:58.76 +06:07:28.3 -- not a known variable star
02:56:00.58 +08:20:54.8 -- not a known variable star
02:56:00.70 +02:31:46.5 -- not a known variable star
02:56:03.69 +08:45:06.3 -- not a known variable star
02:56:10.86 +06:36:37.9 -- not a known variable star
02:56:10.90 +07:26:34.0 -- not a known variable star
02:56:12.32 +09:28:07.5 -- not a known variable star
02:56:12.42 +03:11:47.8 -- not a known variable star
02:56:14.34 +03:34:42.2 -- not a known variable star
02:56:14.59 +03:29:04.4 -- not a known variable star
02:56:14.93 +09:21:05.1 -- not a known variable star
02:56:15.97 +05:56:08.4 -- not a known variable star
02:56:16.75 +02:23:25.3 -- not a known variable star
02:56:17.09 +08:50:58.7 -- not a known variable star
02:56:18.34 +09:18:07.9 -- not a known variable star
02:56:19.18 +05:05:07.9 -- not a known variable star
02:56:19.85 +03:40:48.2 -- not a known variable star
02:56:19.99 +04:20:15.9 -- not a known variable star
02:56:21.01 +06:33:59.0 -- not a known variable star
02:56:21.38 +05:03:29.6 -- not a known variable star
02:56:23.14 +10:02:52.0 -- not a known variable star
02:56:28.13 +07:58:26.8 -- not a known variable star
02:56:29.06 +08:15:07.9 -- not a known variable star
02:56:32.99 +03:38:58.6 -- not a known variable star
02:56:33.58 +03:47:53.5 -- not a known variable star
02:56:33.61 +03:38:56.3 -- not a known variable star
02:56:34.92 +06:52:25.2 -- not a known variable star
02:56:37.16 +01:45:05.7 -- not a known variable star
02:56:38.19 +04:11:58.9 -- not a known variable star
02:56:39.12 +07:45:02.0 -- a known variable star
02:56:40.72 +06:31:51.8 -- not a known variable star
02:56:42.32 +06:42:12.7 -- a known variable star
02:56:43.82 +07:32:34.6 -- not a known variable star
02:56:45.33 +05:17:06.0 -- not a known variable star
02:56:45.63 +08:58:09.7 -- not a known variable star
02:56:46.07 +06:35:13.1 -- not a known variable star
02:56:46.27 +08:58:16.0 -- not a known variable star
02:56:51.75 +07:49:26.7 -- not a known variable star
02:56:54.35 +09:32:25.2 -- not a known variable star
02:56:55.98 +07:27:40.5 -- not a known variable star
02:56:58.22 +10:28:48.8 -- not a known variable star
02:57:00.74 +05:31:44.8 -- not a known variable star
02:57:00.98 +10:18:57.8 -- not a known variable star
02:57:09.71 +09:07:06.7 -- not a known variable star
02:57:10.21 +08:34:18.4 -- not a known variable star
02:57:11.55 +05:55:21.5 -- not a known variable star
02:57:20.36 +06:40:58.5 -- not a known variable star
02:57:21.53 +08:31:15.9 -- not a known variable star
02:57:21.79 +08:31:16.9 -- not a known variable star
02:57:22.15 +05:20:42.6 -- not a known variable star
02:57:24.89 +02:11:05.3 -- not a known variable star
02:57:25.76 +09:21:31.7 -- not a known variable star
02:57:28.61 +09:30:30.4 -- not a known variable star
02:57:29.05 +09:10:22.3 -- not a known variable star
02:57:29.66 +02:53:42.5 -- not a known variable star
02:57:31.75 +09:43:00.6 -- not a known variable star
02:57:35.03 +06:25:56.7 -- not a known variable star
02:57:38.17 +07:10:43.2 -- a known variable star
02:57:41.71 +09:19:29.7 -- not a known variable star
02:57:41.86 +06:06:30.2 -- not a known variable star
02:57:42.56 +05:07:42.3 -- not a known variable star
02:57:44.32 +06:54:45.2 -- not a known variable star
02:57:44.59 +04:12:40.7 -- not a known variable star
02:57:52.14 +08:54:55.3 -- not a known variable star
02:57:54.12 +07:26:05.2 -- not a known variable star
02:57:54.79 +08:10:19.7 -- not a known variable star
02:57:55.29 +08:10:18.8 -- not a known variable star
02:58:00.37 +10:14:03.0 -- not a known variable star
02:58:01.01 +04:03:51.3 -- not a known variable star
02:58:01.54 +03:47:53.2 -- not a known variable star
02:58:04.98 +07:34:12.7 -- not a known variable star
02:58:06.51 +04:15:45.8 -- not a known variable star
02:58:08.35 +08:29:43.4 -- not a known variable star
02:58:12.40 +03:49:34.6 -- not a known variable star
02:58:13.23 +04:21:34.0 -- not a known variable star
02:58:13.45 +03:10:02.9 -- not a known variable star
02:58:31.58 +07:00:19.1 -- not a known variable star
02:58:33.50 +06:32:57.8 -- not a known variable star
02:58:42.40 +05:34:33.7 -- not a known variable star
02:58:43.18 +07:30:54.9 -- not a known variable star
02:58:43.82 +07:30:56.8 -- not a known variable star
02:58:45.92 +05:34:00.3 -- not a known variable star
02:58:50.41 +11:04:11.0 -- not a known variable star
02:58:51.62 +05:04:53.6 -- not a known variable star
02:58:55.18 +03:00:13.0 -- not a known variable star
02:58:59.80 +07:18:50.7 -- not a known variable star
02:58:59.92 +02:05:21.1 -- not a known variable star
02:59:02.74 +01:43:49.5 -- not a known variable star
02:59:09.94 +08:56:18.7 -- not a known variable star
02:59:10.30 +10:42:38.3 -- not a known variable star
02:59:10.44 +08:56:21.6 -- not a known variable star
02:59:14.85 +09:24:35.1 -- not a known variable star
02:59:14.88 +05:43:36.0 -- not a known variable star
02:59:16.27 +01:38:11.8 -- not a known variable star
02:59:19.19 +06:43:39.9 -- a known variable star
02:59:21.12 +01:44:14.1 -- not a known variable star
02:59:21.49 +08:29:43.5 -- not a known variable star
02:59:21.95 +08:05:36.2 -- not a known variable star
02:59:27.39 +06:31:39.1 -- not a known variable star
02:59:29.84 +08:36:25.3 -- not a known variable star
02:59:29.95 +06:20:18.8 -- not a known variable star
02:59:30.72 +01:43:01.3 -- not a known variable star
02:59:30.77 +01:53:09.5 -- not a known variable star
02:59:32.12 +08:46:25.1 -- not a known variable star
02:59:38.01 +04:18:36.6 -- not a known variable star
02:59:40.18 +02:17:19.5 -- not a known variable star
02:59:41.13 +04:05:57.7 -- not a known variable star
02:59:43.92 +08:44:48.3 -- not a known variable star
02:59:45.17 +06:40:31.3 -- not a known variable star
02:59:49.76 +08:39:22.7 -- not a known variable star
02:59:50.18 +08:39:15.4 -- not a known variable star
02:59:54.00 +09:33:22.5 -- not a known variable star
02:59:57.50 +07:58:29.0 -- not a known variable star
02:59:59.96 +07:06:07.6 -- not a known variable star
03:00:01.93 +08:56:49.8 -- not a known variable star
03:00:02.07 +02:56:08.1 -- not a known variable star
03:00:03.90 +06:07:39.1 -- not a known variable star
03:00:04.63 +08:01:20.3 -- not a known variable star
03:00:06.39 +06:38:44.5 -- not a known variable star
03:00:07.89 +06:29:11.5 -- not a known variable star
03:00:08.75 +02:26:30.9 -- not a known variable star
03:00:08.88 +09:09:17.4 -- not a known variable star
03:00:12.62 +02:02:10.0 -- not a known variable star
03:00:13.07 +02:29:49.2 -- not a known variable star
03:00:19.03 +06:55:50.4 -- not a known variable star
03:00:20.03 +01:24:56.7 -- not a known variable star
03:00:26.32 +09:32:43.1 -- not a known variable star
03:00:26.59 +02:10:54.9 -- a known variable star
03:00:29.52 +04:51:26.8 -- not a known variable star
03:00:31.18 +04:10:20.8 -- not a known variable star
03:00:34.21 +10:48:04.6 -- not a known variable star
03:00:36.42 +02:50:13.1 -- not a known variable star
03:00:38.54 +02:34:32.9 -- not a known variable star
03:00:38.56 +04:56:32.1 -- not a known variable star
03:00:49.95 +02:07:34.3 -- not a known variable star
03:00:57.43 +09:20:44.8 -- not a known variable star
03:01:09.19 +08:51:04.5 -- not a known variable star
03:01:09.60 +09:34:27.2 -- not a known variable star
03:01:12.43 +03:59:49.7 -- not a known variable star
03:01:24.55 +07:10:56.7 -- not a known variable star
03:01:26.74 +02:07:53.8 -- not a known variable star
03:01:26.91 +07:51:39.4 -- not a known variable star
03:01:37.89 +01:39:16.5 -- not a known variable star
03:01:39.22 +10:56:36.6 -- a known variable star
03:01:43.48 +09:24:11.1 -- not a known variable star
03:01:45.83 +07:16:41.8 -- not a known variable star
03:01:46.00 +09:26:34.2 -- not a known variable star
03:01:46.89 +09:56:00.0 -- not a known variable star
03:01:49.27 +01:45:00.7 -- not a known variable star
03:01:50.71 +07:44:29.8 -- not a known variable star
03:01:53.16 +08:37:34.2 -- not a known variable star
03:01:54.94 +08:42:56.5 -- not a known variable star
03:01:56.46 +09:21:13.9 -- not a known variable star
03:01:59.53 +03:47:58.8 -- a known variable star
03:02:10.03 +07:51:21.4 -- not a known variable star
03:02:27.39 +09:06:15.2 -- not a known variable star
03:02:29.86 +05:35:05.8 -- not a known variable star
03:02:33.29 +02:04:40.8 -- not a known variable star
03:02:41.61 +07:04:00.7 -- not a known variable star
03:03:01.41 +03:55:34.9 -- not a known variable star
03:03:06.80 +02:01:27.9 -- not a known variable star
03:03:06.96 +10:06:04.1 -- not a known variable star
03:03:15.85 +02:54:13.0 -- not a known variable star
03:03:23.85 +08:38:29.7 -- not a known variable star
03:03:32.99 +08:44:02.0 -- not a known variable star
03:03:33.42 +10:28:16.0 -- not a known variable star
03:03:34.41 +07:25:33.1 -- not a known variable star
03:03:41.88 +01:49:42.3 -- not a known variable star
03:03:44.89 +01:33:56.2 -- not a known variable star
03:03:51.10 +03:51:53.7 -- not a known variable star
03:03:53.64 +09:45:11.1 -- not a known variable star
03:03:54.16 +05:14:27.1 -- not a known variable star
03:04:00.64 +09:39:57.9 -- not a known variable star
03:04:02.95 +08:52:23.5 -- not a known variable star
03:04:17.92 +01:53:40.7 -- not a known variable star
03:04:18.42 +10:06:38.1 -- not a known variable star
03:04:50.92 +08:23:38.9 -- not a known variable star
03:05:03.70 +01:54:25.8 -- not a known variable star
03:05:03.95 +10:43:52.5 -- not a known variable star
03:05:24.21 +08:21:19.0 -- not a known variable star
03:05:38.22 +10:39:28.4 -- not a known variable star
03:05:58.16 +10:47:15.0 -- not a known variable star
03:06:37.50 +08:33:57.7 -- not a known variable star
03:07:00.94 +09:59:55.2 -- not a known variable star
03:07:04.56 +09:22:49.6 -- a known variable star
03:07:08.61 +01:29:33.2 -- not a known variable star
03:07:12.67 +09:25:38.9 -- not a known variable star
03:07:14.37 +10:04:46.6 -- not a known variable star
03:07:24.85 +10:40:47.5 -- not a known variable star
03:08:03.60 +10:31:03.5 -- not a known variable star
03:08:13.12 +10:27:57.6 -- not a known variable star
03:08:30.43 +10:26:48.3 -- a known variable star
03:08:39.46 +10:21:21.9 -- not a known variable star
03:08:49.16 +10:59:45.0 -- not a known variable star
03:08:49.45 +10:59:39.3 -- not a known variable star
03:08:54.76 +09:51:45.2 -- not a known variable star
03:09:08.33 +10:57:07.6 -- not a known variable star
03:09:22.26 +10:48:44.2 -- not a known variable star
03:09:53.66 +10:01:58.2 -- not a known variable star
03:10:06.73 +10:49:44.3 -- not a known variable star
03:13:33.62 +07:37:43.3 -- not a known variable star
03:23:35.75 +09:23:52.0 -- a known variable star
03:23:43.97 +03:53:23.5 -- a known variable star
03:29:25.82 +06:19:09.0 -- a known variable star
03:32:32.81 +07:25:31.8 -- a known variable star
03:36:19.38 +04:35:45.8 -- not a known variable star
03:43:28.67 +07:10:58.8 -- a known variable star
03:43:43.72 +06:55:30.5 -- a known variable star
03:49:27.30 +06:04:41.1 -- a known variable star
Found 224 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
242 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)2461093.65248898 -observatory 500
23:23:24.20 -01:59:19.2 Mercury (-0.1mag)
23:04:23.60 -07:30:16.6 Venus (-3.9mag)
21:42:45.89 -14:53:04.7 Mars (1.1mag)
07:06:06.24 +22:54:19.6 Jupiter (-2.5mag)
00:05:25.79 -01:44:30.6 Saturn (1.0mag)
03:39:59.44 +19:21:43.5 Uranus (5.7mag)
00:03:40.78 -01:01:38.1 Neptune (7.8mag)
20:29:06.93 -22:59:34.4 Pluto (14.5mag)
01:53:26.05 +16:10:07.3 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 22 03:11 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461093.65248898:
07:06:10.24 +22:54:14.3 Io (5.4mag)
07:06:17.71 +22:53:58.6 Europa (5.5mag)
07:05:56.92 +22:54:45.3 Ganymede (4.9mag)
07:06:25.21 +22:53:54.3 Callisto (6.2mag)
07:09:15.16 +23:10:42.8 Himalia (15.0mag)
07:06:07.50 +22:54:19.6 Thebe (15.9mag)
07:08:40.24 +23:19:11.1 Elara (17.0mag)
07:01:39.76 +24:02:18.2 Pasiphae (17.0mag)
07:15:07.13 +22:42:19.4 Carme (18.1mag)
00:05:37.48 -01:44:35.3 Titan (8.8mag)
00:05:31.25 -01:44:29.3 Rhea (10.1mag)
00:05:21.17 -01:45:51.6 Iapetus (11.5mag)
00:05:26.60 -01:44:33.7 Hyperion (14.8mag)
00:07:30.07 -01:31:30.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 22 03:11 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.65248898:
08:45:46.01 +24:30:42.8 JWST
11:35:08.85 +48:30:51.0 Chandra
15:22:38.92 -59:49:29.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 03:11 spacecraft.txt
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Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461093.65248898 at 500
16:59:41.39 -11:03:49.2 17.5mag 10P/Tempel 2
03:37:18.63 +28:57:48.9 18.0mag 123P/West-Hartley
08:23:38.95 +60:42:56.3 18.4mag 124P/Mrkos
21:19:34.21 -07:38:49.1 22.1mag 141P/Machholz
01:21:08.68 +11:54:48.9 17.7mag 145P/Shoemaker-Levy 5
11:02:59.14 +30:34:31.4 17.9mag 164P/Christensen
09:33:08.03 -33:51:48.4 18.0mag 195P/Hill
15:52:03.24 -06:35:53.8 19.2mag 210P/Christensen
18:16:50.89 -21:28:31.2 17.3mag 218P/LINEAR
16:21:33.94 -18:10:56.5 15.2mag 235P/LINEAR
03:56:23.18 +27:44:29.5 17.8mag 240P/NEAT
15:17:37.67 +06:38:25.6 14.8mag 24P/Schaumasse
11:23:31.12 -03:23:09.8 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.88 +27:24:49.9 19.6mag 407P/PanSTARRS-Fuls
17:07:08.56 -11:19:14.3 17.6mag 40P/Vaisala 1
11:02:12.94 -08:51:53.3 16.6mag 43P/Wolf-Harrington
13:25:29.74 -05:49:38.8 20.0mag 489P/Denning
04:34:22.03 +48:34:34.5 17.8mag 493P/2024 Q2 (LONEOS)
06:04:23.14 +47:31:28.8 17.7mag 63P/Wild 1
23:14:36.32 -02:07:32.0 16.2mag 78P/Gehrels 2
20:01:29.92 -22:18:18.9 15.0mag 88P/Howell
15:27:54.62 -29:00:40.5 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.10 -72:35:54.6 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:50.00 +31:12:54.2 18.2mag C/2017 K2 (PanSTARRS)
20:06:38.21 -65:11:38.0 18.1mag C/2020 V2 (ZTF)
17:21:40.38 +04:21:22.6 16.3mag C/2021 G2 (ATLAS)
03:35:40.96 +24:36:42.2 15.8mag C/2022 N2 (PanSTARRS)
09:08:13.27 +29:49:34.3 15.3mag C/2022 QE78 (ATLAS)
08:35:40.57 -06:33:47.3 16.7mag C/2022 R6 (PanSTARRS)
23:53:02.10 +48:26:45.4 18.0mag C/2023 C2 (ATLAS)
09:51:07.87 -20:45:59.6 17.5mag C/2023 F3 (ATLAS)
20:34:45.21 +61:14:30.9 17.3mag C/2023 H5 (Lemmon)
19:34:30.13 -03:24:15.9 16.1mag C/2023 R1 (PANSTARRS)
02:48:55.27 +35:40:34.2 18.5mag C/2023 RS61 (PanSTARRS)
21:01:27.02 +81:19:56.5 18.0mag C/2023 X2 (Lemmon)
06:39:09.79 +63:49:13.4 17.3mag C/2024 A1 (ATLAS)
01:56:45.16 -24:37:50.9 11.2mag C/2024 E1 (Wierzchos)
11:44:58.71 -02:34:51.1 18.1mag C/2024 G2 (ATLAS)
19:28:18.98 +00:39:12.5 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.73 -01:42:52.9 17.7mag C/2024 G6 (ATLAS)
19:53:27.59 +03:15:06.8 15.6mag C/2024 J3 (ATLAS)
02:47:14.60 -31:34:28.8 15.4mag C/2024 T5 (ATLAS)
16:25:06.05 -58:13:48.8 15.6mag C/2025 A6 (Lemmon)
04:50:29.49 +62:14:30.6 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)
15:56:43.44 -13:01:16.1 14.8mag C/2025 L1 (ATLAS)
02:20:14.08 -19:05:58.2 16.7mag C/2025 Q3 (ATLAS)
02:09:34.52 +17:16:44.1 21.2mag C/2025 R2 (SWAN)
22:20:45.87 +17:39:14.7 16.4mag C/2025 R3 (PANSTARRS)
21:46:01.26 -16:50:25.3 21.5mag C/2025 T1 (ATLAS)
03:06:14.39 -20:34:01.3 18.3mag C/2026 A1 (MAPS)
21:03:02.03 +20:55:38.3 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 22 03:13 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
-rw-r--r-- 1 apache apache 6.2K Feb 22 03:11 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 22 03:11 tocp_transients_list.txt