This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2142* 05 46 02.84 +23 20 15.3 11.5 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,2461121.7142,11.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:02.84 +23:20:15.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 12 10.09 +20 36 21.5 11.4 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
VARIABLE_NAME,2461121.7142,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:10.09 +20:36:21.5 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 06 55.95 +25 45 05.1 12.2 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,2461121.7142,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:55.95 +25:45:05.1 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 03 58.72 +19 29 21.5 13.6 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
target,2461121.7142,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:58.72 +19:29:21.5 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 202064086,2461121.7142,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EPIC 202064086 20260322.2142 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:32.19 +22:34:51.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 07 52.33 +18 13 13.5 12.7 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,2461121.7142,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:52.33 +18:13:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 05 25.96 +21 58 39.3 12.8 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
VARIABLE_NAME,2461121.7142,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:25.96 +21:58:39.3 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 17 23.78 +19 07 24.5 13.7 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,2461121.7142,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 13.67CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:23.78 +19:07:24.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 14 28.86 +23 32 58.5 14.1 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,2461121.7142,14.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:28.86 +23:32:58.5 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 33 43.66 +21 07 38.5 14.3 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,2461121.7142,14.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 14.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:43.66 +21:07:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 35 40.02 +25 20 17.4 14.7 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,2461121.7142,14.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 14.72CV 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:40.02 +25:20:17.4 ;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-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 06 00 06.95 +16 48 16.6 13.6 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J060007.16+164817.1,2461121.7142,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J060007.16+164817.1 20260322.2142 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:00:06.95 +16:48:16.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 22 21.74 +18 21 17.1 12.8 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
VARIABLE_NAME,2461121.7142,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260322.2142 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:21.74 +18:21:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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 03 22.2142* 05 47 00.72 +19 35 09.9 11.2 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
ASASSN-V J054700.46+193520.3,2461121.7142,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J054700.46+193520.3 20260322.2142 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:00.72 +19:35:09.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20_00sec_-14_90C_LIGHT_0043_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: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461121.71456448 22.03.2026 05:08:48.371 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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: 7 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): 21961
Objects passed selection criteria: 21948
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 20984.2
Average stars matched: 20566.8 (98.0104 %)
Memory usage VmPeak: 126092 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 00:14:45 CDT 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: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461121.71456448 22.03.2026 05:08:48.371 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 119
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 84 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): 156002
Objects passed selection criteria: 155712
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 143278
Average stars matched: 138939 (96.9713 %)
Memory usage VmPeak: 1927752 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 00:17:45 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> '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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.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: 2461121.71384856
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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
Saving wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits to local_wcs_cache/
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
Saving wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits to local_wcs_cache/
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits'
wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.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 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:17.217 +22:00:01.35
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:14.638 +22:00:38.35
Angular distance between the image centers 0.02 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 05:32:17.217 +22:00:01.35
Second-epoch second image center 05:32:14.638 +22:00:38.35
Angular distance between the image centers 0.01431 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.GzyjkKGLZp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.V9Wm1WiBZv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits &> /tmp/tmp.JupGu6A1pl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.79sDLZQxzJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
The reference image (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat) found
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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 10157 out of 22997 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.956266
a=0.000000 b=1.000000 c=22.956266
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
2.0 pix Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
2.2 pix fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
2.3 pix fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
Limiting magnitude estimates:
15.3 mag. Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.3 mag. Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
15.0 mag. fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
15.0 mag. fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.GzyjkKGLZp (6) ############
Parsing command line arguments...
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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2479, passed=22997
Got 22997 stars (including 20487 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
util/solve_plate_with_UCAC5 got 22997 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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.V9Wm1WiBZv (6) ############
Parsing command line arguments...
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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2545, passed=22806
Got 22806 stars (including 20234 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 22806 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 934.0'
Seting catalog search parameters based on the expected field of view 934.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012972 (46.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010378 (37.4 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 616 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: 2.04"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 661 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.45"
Estimated accuracy of the plate solution: 1.58"
Excluding outliers - 624 stars left (next iteration limit 630)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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.JupGu6A1pl (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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1517, passed=19309
Got 19309 stars (including 17772 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 19309 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.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.79sDLZQxzJ (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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1452, passed=19287
Got 19287 stars (including 17816 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 19287 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.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
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits'
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out31439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31459.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31431_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31431_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:06:08.67 +25:14:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31439_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 31439_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31440_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 31440_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31458_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31458_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:49:03.27 +24:36:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31459_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 31459_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31460_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31460_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:02:40.11 +22:14:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31461_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31461_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:38:44.89 +25:43:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31462_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31462_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:34:14.65 +23:02:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31463_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31463_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:46:41.40 +20:36:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31464_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31464_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:46:55.04 +22:19:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31469_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31469_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:31:11.86 +22:43:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31470_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31470_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:15:47.34 +26:45:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31481_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31481_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:35:44.80 +22:35:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31487_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31487_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:38:35.95 +20:58:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.619 3402713506980589824 084.64986460567 +20.97036120197 12.0204 11.1739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31488_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31488_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:32:28.87 +22:49:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.405 3404126070185863936 083.12035291184 +22.82019185537 12.3053 11.9744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31496_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 31496_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:27:59.32 +20:26:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14186_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 14186_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:55:48.83 +20:10:31.1 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
05:46:02.84 +23:20:15.3
05:12:10.09 +20:36:21.5
05:06:55.95 +25:45:05.1
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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits exists and is non-empty
wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits exists and is non-empty
wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.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 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:17.217 +22:00:01.35
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.563 +21:59:58.39
Second-epoch image center 05:32:14.638 +22:00:38.35
Angular distance between the image centers 0.02 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 05:32:17.217 +22:00:01.35
Second-epoch second image center 05:32:14.638 +22:00:38.35
Angular distance between the image centers 0.01431 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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.y0pyoYontu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits &> /tmp/tmp.dHgyLSqo3u
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits &> /tmp/tmp.Mpbqo3BGsw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.5S4wUZAgjn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
Found non-empty wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
The reference image (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat) found
'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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 10499 out of 167968 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.793970
a=0.000000 b=1.000000 c=22.793970
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 107 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
1.9 pix Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
2.3 pix fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
2.4 pix fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
Limiting magnitude estimates:
15.5 mag. Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.5 mag. Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
15.0 mag. fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
15.0 mag. fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.y0pyoYontu (6) ############
Parsing command line arguments...
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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=21684, passed=167940
Got 167940 stars (including 145994 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat
util/solve_plate_with_UCAC5 got 167940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 932 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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.dHgyLSqo3u (6) ############
Parsing command line arguments...
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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits' -> 'wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=50, blended=21854, passed=169419
Got 169419 stars (including 147299 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat
util/solve_plate_with_UCAC5 got 169419 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 934.0'
Seting catalog search parameters based on the expected field of view 934.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012972 (46.7 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010378 (37.4 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 589 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: 2.15"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.75"
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 643 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.74"
Estimated accuracy of the plate solution: 1.56"
Excluding outliers - 601 stars left (next iteration limit 606)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits -region wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.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.Mpbqo3BGsw (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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=12762, passed=120769
Got 120769 stars (including 107805 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 120769 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 931 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.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.5S4wUZAgjn (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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.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_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=12430, passed=118323
Got 118323 stars (including 105702 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 118323 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 930 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.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
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/wcs_Tau-04-Q1b1x1_2025-12-23_01-27-56_20.00sec_-15.00C_LIGHT_0379.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-07-46_20.00sec_-14.90C_LIGHT_0043.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Tau-04-Q1b1x1_001001_TTUQ1b1x1_30095_yISdLkOh/wcs_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044.fits
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out193676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out193689.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out194008.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out126539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out147723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194331.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 8s
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Considering the candidate 193676_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193676_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:37:12.00 +16:56:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 2.482 3397027386895771392 084.30021079140 +16.94085371687 14.3625 13.7423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193680_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193680_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:00:55.03 +26:26:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193683_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193683_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:40:38.43 +25:12:44.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 193685_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193685_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:56:49.47 +24:12:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 2.914 3427949570880792192 089.20524571409 +24.20780392965 14.5711 13.9331 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193689_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193689_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:57:14.08 +26:20:58.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)
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Considering the candidate 193696_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193696_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:38:14.72 +25:05:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.205 3440767608715684864 084.56107564270 +25.08860096864 14.0915 13.4267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193710_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193710_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:56:26.02 +18:57:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193716_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193716_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:38:21.21 +23:43:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193718_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193718_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:18:55.52 +23:05:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.836 3415597725971724800 079.73085061352 +23.09159525902 13.8631 13.1047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193725_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 193725_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 193730_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193730_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:52:15.32 +23:56:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193734_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 193734_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 193745_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193745_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:46:02.78 +23:20:16.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193746_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193746_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:12:10.11 +20:36:21.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193760_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193760_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:06:55.97 +25:45:05.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193783_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193783_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:43:34.71 +25:27:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193784_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193784_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:05:45.98 +26:25:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193785_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193785_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:20:11.80 +19:34:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 1.517 3401770297804621312 080.04874480294 +19.57147341607 12.3819 11.5616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.517#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193786_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 193786_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 193788_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193788_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:04:13.43 +25:24:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193793_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193793_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 193794_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193794_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:31:11.00 +20:10:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193799_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 193799_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 193809_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193809_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:29:17.25 +18:20:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.299 3400466586252024192 082.32153519349 +18.33785597679 12.9437 12.4305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.299#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193812_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193812_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:48:27.21 +20:53:27.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193827_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193827_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:49:44.92 +24:06:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193828_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193828_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:58:09.45 +21:58:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193830_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193830_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:56:13.25 +17:26:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.736 3350012750729673984 089.05540871551 +17.43493359343 13.3824 12.8421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.736#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193841_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193841_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:55:14.60 +20:28:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193842_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193842_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:51:41.48 +23:14:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193845_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193845_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:41:53.49 +18:32:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.155 3399115428197361920 085.47249163523 +18.54992025856 13.2513 12.4203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193847_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193847_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:10:48.66 +25:09:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193859_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193859_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:54:36.51 +18:27:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.327 3398536466605483136 088.65173698108 +18.46549234676 13.0481 12.0522 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 193865_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193865_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:20:20.50 +25:08:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193880_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193880_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:59:41.59 +19:52:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193882_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193882_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:37:40.15 +22:58:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193886_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193886_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:00:17.16 +25:10:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193890_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193890_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:43:36.64 +25:27:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193892_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193892_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:06:02.89 +26:31:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.583 3430108221444418944 091.51161592595 +26.51938654656 13.9144 13.5753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193909_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193909_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:50:27.68 +18:02:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193913_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193913_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:53:58.65 +21:51:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193914_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193914_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:57:10.45 +21:28:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193915_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193915_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:39:27.59 +21:47:28.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193920_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193920_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:36:21.07 +24:22:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193922_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 193922_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 193927_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193927_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:47:20.97 +23:52:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193928_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193928_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:17:30.52 +20:09:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193931_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193931_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:36:40.73 +18:53:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193933_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193933_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:47:37.33 +23:38:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193935_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193935_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:58:05.50 +24:37:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193946_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193946_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:37:31.28 +19:46:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.599 3402478215789164544 084.37989169579 +19.77012858654 13.6040 12.7386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193952_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193952_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:27:21.90 +17:17:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193954_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193954_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:37:16.86 +17:19:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.083 3397430529706392576 084.32003573678 +17.33402616171 13.6884 12.8255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193956_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193956_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:03:16.11 +16:56:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193960_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193960_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:01:09.95 +22:31:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193967_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193967_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:27:58.76 +21:26:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193968_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193968_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:57:24.38 +18:20:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193975_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193975_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:33:24.68 +18:32:32.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193978_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193978_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:48:40.54 +18:15:24.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193990_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193990_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:37:56.40 +22:27:00.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193999_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 193999_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:54:42.53 +17:25:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194008_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194008_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:49:44.55 +20:13:14.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)
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Considering the candidate 194014_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194014_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:08:52.83 +19:50:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194038_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194038_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:34:12.08 +25:35:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194044_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194044_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:38:24.17 +26:07:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.010 3440993523995236480 084.60042564509 +26.12559162081 14.0576 13.0835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194070_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194070_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:54:10.40 +24:05:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194074_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 194074_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194083_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194083_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:32:34.41 +21:00:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194088_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194088_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:19:43.70 +26:10:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194100_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194100_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:46:04.92 +19:23:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194102_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194102_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:38:22.79 +21:36:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 2.163 3403006737286022272 084.59480505406 +21.61522270392 14.2858 13.4349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194104_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194104_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:39:50.00 +19:23:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 4.228 3399453218783579648 084.95752341588 +19.39930871915 14.5647 14.0076 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194110_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194110_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:31:04.92 +23:13:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.649 3416166276561542016 082.77030613945 +23.23136640704 14.2133 13.8115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194119_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194119_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:54:46.01 +22:03:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 0.159 3424096572896914944 088.69174685449 +22.06386305075 14.3381 13.5793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194126_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194126_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:59:10.44 +25:14:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 0.993 3429572278244517632 089.79324372427 +25.24198266584 14.5466 13.9829 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 194133_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194133_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:40:43.55 +27:00:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194140_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194140_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:29:43.09 +22:48:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194152_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 194152_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 194157_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194157_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:48:50.02 +24:34:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.51, MAG_FAINT_SEARCH_LIMIT=15.49)GAIADR2_OUTPUT=# 0.996 3427801858363621248 087.20842650995 +24.58230431925 14.6172 14.0136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194163_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194163_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:01:46.68 +26:34:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.749 3429961917677223552 090.44462367470 +26.57200551183 14.3169 13.4620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194165_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194165_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:41:48.26 +21:43:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194195_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194195_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:04:35.02 +21:26:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194203_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194203_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:00:28.36 +26:20:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194234_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194234_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:50:09.96 +24:44:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 0.768 3428182255027499264 087.54127222104 +24.73591309675 14.7575 14.1315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194238_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194238_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:56:34.47 +17:16:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 2.118 3349819786438649728 089.14324003899 +17.27551487022 14.7487 14.1993 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 194244_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194244_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:59:44.30 +25:34:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 0.652 3429616705386100096 089.93441733334 +25.57621317387 14.4655 13.5116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194246_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194246_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:45:57.46 +23:43:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 1.639 3427654386366217600 086.48892148751 +23.72948448301 14.4888 13.8933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194247_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194247_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:35:51.68 +22:16:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 3.386 3403805910440802304 083.96472197602 +22.28191802622 14.9757 14.3705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194248_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194248_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:57:39.84 +24:34:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194251_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194251_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:03:14.20 +24:42:04.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)
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Considering the candidate 194281_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194281_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:55:41.26 +24:40:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 2.822 3428040143150694656 088.92193286827 +24.68153386563 13.3084 11.9252 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194298_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194298_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:59:49.08 +24:08:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.993 3424957696660517120 089.95438805174 +24.14895055720 14.6433 13.8901 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 194312_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194312_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:01:14.12 +21:33:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.670 3423224900694158208 090.30834470451 +21.56246180466 14.6168 13.8675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194331_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 194331_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 194338_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194338_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:41:07.90 +20:46:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 0.740 3402666816392874368 085.28270496284 +20.76686129308 14.8207 14.1970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194345_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194345_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:05:03.20 +26:12:55.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)
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Considering the candidate 194348_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194348_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:05:33.20 +24:17:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 0.932 3426239486700611456 091.38819209314 +24.29769687748 14.5718 14.1370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194364_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 194364_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:47:59.93 +26:04:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 1.316 3429262181604342400 086.99933996159 +26.07140510166 14.7558 14.1984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 46902_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 46902_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 06:01:26.85 +23:51:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74248_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 74248_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:37:26.67 +22:20:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07287_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 07287_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:15:47.37 +26:45:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154292_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 154292_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 82933_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 82933_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:53:50.56 +21:45:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05101_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 05101_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks
**** FOUND 05:52:51.76 +26:47:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126539_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 126539_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 147723_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
Preparing report for the candidate 147723_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
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Considering the candidate 111854_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044
The candidate 111854_fd_Tau-04-Q1b1x1_2026-03-22_00-08-48_20.00sec_-15.00C_LIGHT_0044 did not pass the final checks