This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5
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 22.1984* 05 46 02.15 +23 20 15.6 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,2461121.6984,11.52,0.05,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 20260322.1984 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:02.15 +23:20:15.6 ;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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 12 09.00 +20 36 19.0 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,2461121.6984,11.44,0.05,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 20260322.1984 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:09.00 +20:36:19.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 06 55.01 +25 45 04.3 12.3 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,2461121.6984,12.34,0.05,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 20260322.1984 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:55.01 +25:45:04.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 07 51.19 +18 13 11.1 12.6 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
VARIABLE_NAME,2461121.6984,12.61,0.05,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 20260322.1984 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:51.19 +18:13:11.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 05 24.79 +21 58 39.1 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,2461121.6984,12.84,0.05,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 20260322.1984 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:24.79 +21:58:39.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.1984 2461121.6984 13.79 05:47:20.96 +23:52:58.4
184.52124 -2.29232 galactic Tau Second-epoch detections are separated by 1.2" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J086.8387+23.8837 | 05:47:20.96 +23:52:58.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: F0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.1984* 05 47 20.96 +23 52 58.4 13.8 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
ATO J086.8387+23.8837,2461121.6984,13.79,0.05,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
ATO J086.8387+23.8837 20260322.1984 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:20.96 +23:52:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 39 21.41 +17 46 54.9 13.8 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
target,2461121.6984,13.76,0.05,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 20260322.1984 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:21.41 +17:46:54.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 17 22.65 +19 07 23.8 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,2461121.6984,13.68,0.05,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 20260322.1984 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:22.65 +19:07:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 14 27.87 +23 32 59.1 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,2461121.6984,14.12,0.05,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 20260322.1984 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:27.87 +23:32:59.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.1984 2461121.6984 14.32 05:52:47.33 +17:41:57.1
190.49705 -4.35773 galactic Tau Second-epoch detections are separated by 1.8" and 8.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J088.1967+17.7000 | 05:52:48.07 +17:41:26.0 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.1984* 05 52 47.33 +17 41 57.1 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
ATO J088.1967+17.7000,2461121.6984,14.32,0.05,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
ATO J088.1967+17.7000 20260322.1984 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:47.33 +17:41:57.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 33 42.79 +21 07 36.9 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,2461121.6984,14.34,0.05,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 20260322.1984 14.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:42.79 +21:07:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 35 38.99 +25 20 20.0 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,2461121.6984,14.74,0.05,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 20260322.1984 14.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:38.99 +25:20:20.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 13 56.79 +19 10 10.4 14.6 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
VARIABLE_NAME,2461121.6984,14.62,0.05,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
VARIABLE_NAME 20260322.1984 14.62CV 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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:56.79 +19:10:10.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 53 50.52 +21 45 08.1 12.6 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
NSVS J0553506+214506,2461121.6984,12.62,0.05,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
NSVS J0553506+214506 20260322.1984 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:50.52 +21:45:08.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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 22.1984* 05 22 20.85 +18 21 14.0 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,2461121.6984,12.75,0.05,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 20260322.1984 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:20.85 +18:21:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q1b1x1_2025-12-23_01-27-09_20_00sec_-15_00C_LIGHT_0378_fits__*pix.png resample_wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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_2026-03-21_23-46-01_20_00sec_-15_00C_LIGHT_0020_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_2026-03-21_23-45-03_20_00sec_-14_90C_LIGHT_0019_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: 2461121.69874470 22.03.2026 04:46:01.542 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
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: 6 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): 22214
Objects passed selection criteria: 22200
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: 21355.8
Average stars matched: 20908.8 (97.9069 %)
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 Sat Mar 21 23:47:50 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: 2461121.69874470 22.03.2026 04:46:01.542 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 151
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: 77 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): 158432
Objects passed selection criteria: 158135
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 148760
Average stars matched: 144183 (96.9236 %)
Memory usage VmPeak: 1980756 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 Sat Mar 21 23:50:27 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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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: 2461121.69807735
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_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits'
wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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 05:32:18.573 +22:00:00.48
Angular distance between the image centers 0.00 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 05:32:21.766 +22:00:00.55
Angular distance between the image centers 0.01 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 05:32:18.573 +22:00:00.48
Second-epoch second image center 05:32:21.766 +22:00:00.55
Angular distance between the image centers 0.01234 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.TVnVdmV7Uy
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.8pgx7zn5P6
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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.uKXzj3qpS3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.iFrycrIp2i
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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 22 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
2.1 pix fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
2.1 pix fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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
15.1 mag. fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
15.1 mag. fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (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.TVnVdmV7Uy (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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/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.8pgx7zn5P6 (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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/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.uKXzj3qpS3 (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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.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_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1672, passed=20087
Got 20087 stars (including 18392 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 20087 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 938 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: 0.36"
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 938 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: 0.37"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.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.iFrycrIp2i (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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1661, passed=20026
Got 20026 stars (including 18339 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 20026 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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: 0.37"
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 936 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: 0.37"
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_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/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_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits'
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out31436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31437.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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
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Considering the candidate 31428_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31428_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:44:17.54 +22:41:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 1.898 3403511447482409856 086.07312377679 +22.69774810044 11.6053 11.2076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31429_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31429_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:06:08.67 +25:14:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31436_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 31436_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
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Considering the candidate 31437_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 31437_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31444_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31444_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:50:17.01 +17:03:33.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31446_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31446_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:02:40.06 +22:14:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31452_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31452_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:50:06.36 +21:08:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 1.312 3400113441157674112 087.52657149478 +21.14055261474 12.1519 11.6658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31456_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31456_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:53:07.25 +20:47:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31457_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31457_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:15:47.35 +26:45:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31459_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31459_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:36:54.95 +20:50:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31460_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31460_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:35:22.02 +20:48:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.406 3402810848119383168 083.84175389792 +20.80072399780 11.9167 11.1159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31463_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31463_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:38:44.86 +25:43:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31468_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31468_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:40:07.78 +21:25:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31469_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31469_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:53:43.45 +22:38:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31470_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31470_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:30:54.00 +21:37:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31473_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31473_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:44:16.83 +24:27:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31475_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31475_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:34:39.47 +23:44:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.133 3404573502698643968 083.66442075200 +23.74897937932 12.2202 11.6990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 31477_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31477_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:45:43.15 +23:38:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.946 3427646994726031872 086.42990310766 +23.63774214694 12.3418 11.8425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31478_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31478_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:27:24.07 +22:55:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31491_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31491_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:27:59.31 +20:26:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 2.084 3402071014232819584 081.99711767763 +20.44207876033 12.0182 11.1365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31500_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 31500_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:24:38.45 +20:52:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14186_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 14186_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:55:48.83 +20:10:31.4 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
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 ####
05:46:02.15 +23:20:15.6
05:12:09.00 +20:36:19.0
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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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 05:32:18.573 +22:00:00.48
Angular distance between the image centers 0.00 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 05:32:21.766 +22:00:00.55
Angular distance between the image centers 0.01 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 05:32:18.573 +22:00:00.48
Second-epoch second image center 05:32:21.766 +22:00:00.55
Angular distance between the image centers 0.01234 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.aSjSSDszL8
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.3cwMMjcWzT
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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.r5GHVRHRTf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.WnDKH1LBn0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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 146 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
2.2 pix fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
2.2 pix fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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
15.1 mag. fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
15.1 mag. fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.4 (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.aSjSSDszL8 (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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/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.3cwMMjcWzT (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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/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.r5GHVRHRTf (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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.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_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=13989, passed=130861
Got 130861 stars (including 116675 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 130861 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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: 0.35"
Estimated accuracy of the plate solution: 0.35"
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_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.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.WnDKH1LBn0 (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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=13946, passed=130235
Got 130235 stars (including 116082 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat
util/solve_plate_with_UCAC5 got 130235 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 929 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/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_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-45-03_20.00sec_-14.90C_LIGHT_0019.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.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_2026-03-21_CI_Tau-04-Q1b1x1_234641_TTUQ1b1x1_17650_p7mvx5x5/wcs_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020.fits
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out193665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193674.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194372.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194418.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out126539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82933.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 7s
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Considering the candidate 193665_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193665_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:37:49.21 +21:44:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 0.527 3403012436707056512 084.45489835788 +21.73947742034 14.9487 14.3584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193671_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193671_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:50:43.01 +21:29:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 0.637 3400129555874878208 087.67907127746 +21.49979383494 15.0331 14.4078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193674_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193674_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:56:56.64 +22:06:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.711 3424109320360072064 089.23576860993 +22.10765901502 15.0423 14.4289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.711#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193678_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193678_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:33:19.63 +21:46:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.799 3403807422269572224 083.33192313261 +21.77887360838 14.8996 14.3707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193687_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193687_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:51:22.84 +20:48:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 3.771 3399902231845426816 087.84455824658 +20.80274069657 14.8462 14.0966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193688_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193688_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:54:45.71 +20:47:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.559 3423111616638063872 088.69031936076 +20.79088539956 14.4633 13.5782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193695_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193695_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:29:19.42 +18:19:25.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)
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Considering the candidate 193702_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193702_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:05:59.10 +25:07:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 2.086 3426565869858314752 091.49585938444 +25.12654226279 14.8011 14.4484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193718_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193718_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:38:21.22 +23:43:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193727_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193727_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:00:55.08 +26:26:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.128 3429954216797430144 090.22884109921 +26.44926859466 14.4969 13.7630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193729_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193729_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:04:14.39 +24:17:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 0.571 3426242407278485504 091.06005174545 +24.29535620962 14.7600 14.2730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193735_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193735_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:39:59.68 +25:04:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.588 3428783241210821248 084.99824501750 +25.07188750882 14.2448 13.5754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193738_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193738_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:05:13.11 +26:02:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 2.075 3430058532963351936 091.30400608723 +26.04351267278 14.0932 13.7466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193743_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193743_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:59:50.41 +18:06:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.061 3350254815085214336 089.95974126760 +18.10534372664 14.2161 13.5286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193747_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193747_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:50:30.09 +22:01:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.104 3424227174263376256 087.62572272468 +22.01965428476 13.9157 13.3342 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193749_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193749_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:17:26.62 +18:34:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193759_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193759_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:05:58.53 +25:07:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193760_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193760_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:09:20.66 +18:14:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193762_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193762_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:06:47.74 +17:04:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.884 3394977794140845568 076.69848478319 +17.06793277362 13.4548 12.8004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193765_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193765_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:52:15.29 +23:56:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193772_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193772_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:04:34.95 +19:56:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.098 3374817320734101760 091.14562557800 +19.94030507633 12.9248 12.0174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193775_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193775_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:44:36.01 +18:12:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193782_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193782_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:46:02.11 +23:20:16.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193783_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193783_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:12:09.03 +20:36:19.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 193800_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193800_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:36:38.08 +25:43:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193802_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 193802_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
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Considering the candidate 193818_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193818_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:05:46.00 +26:25:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193820_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 193820_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
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Considering the candidate 193825_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193825_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:43:34.72 +25:27:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193830_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193830_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:04:13.43 +25:24:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193833_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193833_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:05:41.78 +23:02:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.261 3418398147728086400 076.42376771404 +23.04055419150 12.6924 12.1336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193846_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 193846_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
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Considering the candidate 193856_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193856_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:48:27.24 +20:53:28.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193863_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193863_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:32:03.08 +18:33:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.212 3400807606659771136 083.01218604634 +18.56616114258 12.8533 12.0230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193872_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193872_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:49:45.00 +24:06:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193879_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193879_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:58:09.51 +21:58:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193897_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193897_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:02:40.99 +18:32:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 0.602 3350382255354937600 090.67061542871 +18.53647946983 13.4548 12.9479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193902_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193902_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:10:48.65 +25:09:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193916_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193916_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:00:17.25 +25:10:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193920_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193920_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:53:58.67 +21:51:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193921_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193921_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:59:41.54 +19:52:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193925_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193925_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:20:20.47 +25:08:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193940_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193940_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:49:12.05 +19:49:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193941_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193941_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:43:36.69 +25:27:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193942_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193942_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:58:05.50 +24:37:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.362 3427999289421997312 089.52351767214 +24.62064616943 13.7976 13.1199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193944_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193944_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:17:30.55 +20:09:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193948_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193948_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:04:11.89 +25:12:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193956_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 193956_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193958_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193958_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:50:27.55 +18:02:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193959_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193959_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:36:40.79 +18:53:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193966_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193966_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:23:52.03 +20:00:17.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193967_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193967_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:45:37.71 +19:23:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.181 3399266989001794944 086.40826067319 +19.38777347468 13.7018 12.9944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.181#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193969_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 193969_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193982_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193982_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:36:21.05 +24:22:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.658 3416719880666498048 084.08691634126 +24.36710153197 13.7809 13.1577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193983_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 193983_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193984_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193984_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:59:55.93 +22:05:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193986_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193986_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:48:40.43 +18:15:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 3.680 3398388513572526848 087.16797631017 +18.25785855461 13.9100 13.2916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193991_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193991_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:54:24.81 +18:35:02.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193999_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 193999_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:01:09.90 +22:31:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.754 3424465179874067584 090.29102767795 +22.52745787904 13.3307 12.1221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194003_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194003_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:35:41.00 +20:49:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194005_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194005_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:27:20.59 +17:15:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.776 3400229164754794880 081.83499945679 +17.25809395048 13.7219 12.8729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194023_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194023_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:57:24.48 +18:20:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194028_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194028_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:27:21.88 +17:17:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194048_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194048_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:36:30.71 +25:57:49.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194061_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194061_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:22:01.69 +18:15:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194063_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194063_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:08:52.78 +19:50:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194064_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194064_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:33:24.53 +18:32:31.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194070_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194070_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:37:56.39 +22:27:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.293 3404187097378396544 084.48464805844 +22.45029973669 13.4733 12.4391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194076_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194076_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:47:31.35 +17:38:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194092_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194092_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:34:57.27 +18:36:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.579 3397817179840325504 083.73850326374 +18.61636026558 14.2138 13.4265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194094_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194094_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:08:59.39 +20:30:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 4.953 3408088748747812608 077.24602187895 +20.51009298652 14.1986 13.4921 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194099_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194099_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:22:00.67 +18:15:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194121_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 194121_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194125_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194125_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:46:04.90 +19:23:47.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194133_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194133_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:02:57.10 +19:31:47.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194142_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194142_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:37:19.80 +26:53:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.171 3441286092872200448 084.33219519558 +26.89726567942 13.8633 12.8095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194150_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194150_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:17:33.70 +24:02:01.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194153_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194153_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:32:34.58 +21:00:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194159_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194159_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:34:20.07 +20:16:52.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194172_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194172_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:25:13.13 +26:28:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194176_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194176_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:54:10.44 +24:05:10.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194186_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 194186_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194190_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194190_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:49:26.62 +26:47:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194192_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194192_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:05:49.11 +26:17:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194204_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194204_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:42:14.04 +25:29:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194207_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194207_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:58:55.55 +26:28:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 2.851 3429987653121082240 089.73070839116 +26.47278111666 14.3202 13.4309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194226_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194226_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:44:00.98 +18:08:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194232_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194232_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:49:31.19 +23:26:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194236_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194236_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:44:15.62 +24:09:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.632 3428432978038550912 086.06489420509 +24.16368280039 14.5952 14.0072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194243_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 194243_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
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Considering the candidate 194246_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194246_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:33:18.26 +21:13:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 1.505 3403634244890383360 083.32601797382 +21.22602462422 14.6016 14.1289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194249_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194249_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:49:31.16 +20:38:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194272_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194272_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:29:43.15 +22:48:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 4.535 3404114319154223232 082.42916987290 +22.80489962123 14.5741 13.9192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194273_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194273_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:33:33.76 +21:42:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194276_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194276_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:48:08.70 +22:18:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.786 3427258802698790272 087.03626836868 +22.31132930143 14.6151 13.9460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194279_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194279_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:23:41.68 +26:14:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194286_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194286_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:02:12.61 +25:50:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 1.417 3429711641343830912 090.55215054846 +25.84078713794 14.5273 13.9934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194287_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194287_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:44:37.71 +20:42:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.51, MAG_FAINT_SEARCH_LIMIT=15.49)GAIADR2_OUTPUT=# 3.441 3400015103585172224 086.15631801015 +20.70789194642 14.0739 13.0038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194303_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194303_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:35:07.72 +21:01:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 1.437 3402869985527119232 083.78258759964 +21.03137423123 14.7381 14.0875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194304_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194304_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:34:52.50 +19:45:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 3.708 3401041257170405376 083.71791158503 +19.76530112724 14.6113 14.0522 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194326_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194326_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:39:00.75 +19:30:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 2.321 3399470192494352384 084.75295413434 +19.50126312560 15.1302 14.5347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194329_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194329_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:06:04.19 +24:41:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 1.708 3426350090698822656 091.51725909102 +24.69377196213 14.1462 13.1979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194349_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194349_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:18:58.95 +23:04:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 4.177 3415594702314748288 079.74641029618 +23.07954691209 14.3597 13.5634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194351_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194351_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:37:07.93 +24:15:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.59, MAG_FAINT_SEARCH_LIMIT=15.57)GAIADR2_OUTPUT=# 3.617 3404706234368903424 084.28249282005 +24.25353787420 14.6492 13.9749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194363_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194363_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:04:34.98 +21:26:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.172 3423384295521734144 091.14571161467 +21.43454573839 14.2099 13.1734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194372_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194372_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:48:31.91 +24:20:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.572 3427788698583895168 087.13252737480 +24.33549659903 14.6520 14.1372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194374_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194374_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:45:26.12 +23:37:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 2.166 3427647273900431488 086.35817668185 +23.61855512974 14.6385 13.7693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194375_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194375_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:53:48.51 +24:28:09.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)
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Considering the candidate 194393_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194393_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:00:28.33 +26:20:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 2.210 3429929890102493696 090.11817757243 +26.33912935432 14.6205 13.9388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194402_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194402_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:52:08.35 +18:47:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 3.354 3398618375925478144 088.03420670902 +18.78666583150 14.6788 14.0716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194415_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194415_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:39:58.47 +24:31:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.263 3428679646600120064 084.99341417867 +24.52804387550 14.6047 13.9599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194418_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194418_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:01:34.85 +24:58:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 2.379 3426523950974920448 090.39468584920 +24.97126655842 14.5168 13.8753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194425_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194425_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:00:44.48 +25:50:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 2.150 3429720265638273408 090.18477574657 +25.83885170721 14.7208 14.1218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194429_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194429_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:32:04.91 +22:14:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 3.925 3404024781973938816 083.02151561988 +22.23761969229 15.0434 14.6459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194447_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194447_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:03:05.70 +24:18:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 1.500 3426409429967993472 090.77333187752 +24.30108506322 14.5760 14.0214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194460_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194460_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:52:12.67 +21:25:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 1.218 3423956488244020864 088.05267862895 +21.42548391557 14.8492 14.2709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194466_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194466_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:58:49.84 +17:06:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 1.198 3349757973269556480 089.70735102411 +17.10722412321 14.5325 13.9477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194470_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194470_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:29:30.19 +26:11:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 2.459 3417925701324717952 082.37510515853 +26.19346179612 14.6760 13.8537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194471_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194471_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:58:17.13 +25:52:16.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)
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Considering the candidate 194472_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194472_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:57:10.52 +20:40:40.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)
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Considering the candidate 194473_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194473_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:05:31.23 +23:56:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 1.213 3426195368797230464 091.37978339990 +23.94795996056 14.4919 13.8695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.213#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194484_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 194484_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
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Considering the candidate 194495_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194495_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:44:25.17 +20:00:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.918 3399556950833537152 086.10501139498 +20.00446161413 14.7293 13.9746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194499_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194499_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:57:39.82 +24:34:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.724 3428000320214189568 089.41551525232 +24.57155973163 14.5546 14.1066 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.724#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194507_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194507_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:42:56.85 +24:23:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.435 3428498673857942528 085.73656120040 +24.39652758529 15.0585 14.4206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194511_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194511_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:34:31.79 +22:21:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 2.034 3403862496631593984 083.63208152342 +22.36336152886 14.5735 13.8475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194522_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194522_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:45:16.79 +20:31:33.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)
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Considering the candidate 194547_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194547_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:49:42.08 +25:24:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.341 3428994416164355328 087.42504281971 +25.40032007967 14.6419 13.9991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194554_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194554_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:57:44.21 +19:58:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.438 3398804811863739008 089.43406786430 +19.97690473099 14.6818 14.0696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194555_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194555_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:46:29.27 +25:02:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 4.523 3428628416230753792 086.62068678904 +25.04627610290 15.1210 14.3878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194559_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194559_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:46:29.81 +26:39:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 2.065 3429445280351956864 086.62364542810 +26.65263667600 14.6580 13.7922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194562_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194562_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:50:47.19 +23:30:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 2.029 3427503478395446144 087.69610295702 +23.51304738972 14.8583 14.3092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194576_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 194576_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
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Considering the candidate 194584_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194584_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:54:11.50 +17:52:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 1.919 3350100432485574144 088.54775177911 +17.87887062437 14.7913 14.2796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194588_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194588_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:42:19.27 +19:15:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 2.730 3399223485278081664 085.58054061673 +19.26722094472 14.8248 14.1327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194590_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194590_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:37:11.98 +26:58:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 2.049 3441299463105749248 084.29928757877 +26.97487655663 14.7834 14.1681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194675_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194675_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:30:21.13 +20:34:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.557 3402087648644419200 082.58765749611 +20.57643441990 14.7120 14.0324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194680_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194680_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:24:21.91 +20:15:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 2.632 3402009029265380096 081.09156980902 +20.26462743585 14.8294 13.9559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194684_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 194684_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:15:36.64 +22:41:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 1.432 3415477020211289984 078.90244911697 +22.69889897068 14.9544 14.2890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 46902_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 46902_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 06:01:26.90 +23:51:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74248_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 74248_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:37:26.68 +22:20:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07287_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 07287_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 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 82933_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 82933_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
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Considering the candidate 05101_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 05101_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks
**** FOUND 05:52:51.78 +26:47:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126539_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
Preparing report for the candidate 126539_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
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Considering the candidate 111854_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020
The candidate 111854_fd_Tau-04-Q1b1x1_2026-03-21_23-46-01_20.00sec_-15.00C_LIGHT_0020 did not pass the final checks