This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd
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 30.1113* 05 21 45.74 +20 54 41.4 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,2461129.6113,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1113 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:45.74 +20:54:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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 30.1113* 05 52 12.91 +23 17 08.0 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3427434793278648704,2461129.6113,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3427434793278648704 20260330.1113 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:12.91 +23:17:08.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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 30.1113* 05 15 12.92 +25 58 00.2 12.4 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,2461129.6113,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1113 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:12.92 +25:58:00.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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 30.1113* 05 17 47.15 +18 30 01.7 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,2461129.6113,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1113 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:47.15 +18:30:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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 30.1113* 05 15 26.40 +22 06 50.6 13.0 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461129.6113,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1113 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:26.40 +22:06:50.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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 30.1113* 05 27 43.02 +19 11 47.1 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
VARIABLE_NAME,2461129.6113,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1113 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:43.02 +19:11:47.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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 30.1113* 05 18 00.41 +18 21 18.2 11.7 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
ASAS J051800+1821.3,2461129.6113,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J051800+1821.3 20260330.1113 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:00.41 +18:21:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20_00sec_-10_00C_LIGHT_0055_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20_00sec_-15_00C_LIGHT_0038_fits__*pix.png resample_wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20_00sec_-10_00C_LIGHT_0054_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: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
First image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Last image: 2461129.61164219 30.03.2026 02:40:35.885 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.67
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: 4 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): 18559
Objects passed selection criteria: 18470
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 12956.5
Average stars matched: 12136.2 (93.6692 %)
Memory usage VmPeak: 123508 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 21:46:57 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: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
First image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Last image: 2461129.61164219 30.03.2026 02:40:35.885 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 144
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 30 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): 134882
Objects passed selection criteria: 134549
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 96822
Average stars matched: 90318 (93.2825 %)
Memory usage VmPeak: 2355436 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 21:49:17 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/TTUQ2b1x1/TTUQ2_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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.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: 2461129.61102775
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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
Saving wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits'
wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.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 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:18.915 +22:00:59.54
Angular distance between the image centers 0.02 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 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:22.059 +22:00:32.86
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 05:32:18.915 +22:00:59.54
Second-epoch second image center 05:32:22.059 +22:00:32.86
Angular distance between the image centers 0.01423 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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.hcaDAS8nZ5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.PNHARVyigL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits &> /tmp/tmp.YGeZTMAhDH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits &> /tmp/tmp.VtWXXjTxQU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits) and catalog (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat) found
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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 10254 out of 23525 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.945337
a=0.000000 b=1.000000 c=22.945337
From vast_summary.log: estimated ref. image limiting mag.: -7.67
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
2.3 pix Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
2.5 pix fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
2.5 pix fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
Limiting magnitude estimates:
15.3 mag. Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
15.3 mag. Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
14.1 mag. fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
14.0 mag. fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.3 (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.hcaDAS8nZ5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2582, passed=23525
Got 23525 stars (including 20915 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 23525 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
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_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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.PNHARVyigL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2595, passed=23514
Got 23514 stars (including 20891 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 23514 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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.YGeZTMAhDH (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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=617, passed=8745
Got 8745 stars (including 8113 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 8745 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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: 0.65"
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.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.VtWXXjTxQU (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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=588, passed=8560
Got 8560 stars (including 7966 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat
util/solve_plate_with_UCAC5 got 8560 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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: 0.65"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 927 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits'
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32102_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 32102_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:09:43.14 +23:02:03.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18021_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 18021_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:35:58.46 +24:44:53.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07693_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 07693_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:55:48.79 +20:10:33.8 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.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 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:18.915 +22:00:59.54
Angular distance between the image centers 0.02 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 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:22.059 +22:00:32.86
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 05:32:18.915 +22:00:59.54
Second-epoch second image center 05:32:22.059 +22:00:32.86
Angular distance between the image centers 0.01423 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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.rpC44dR1EI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.BYePc82TiC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits &> /tmp/tmp.4chFXe6ow7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits &> /tmp/tmp.I3FEe20NlB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
Found non-empty wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
The reference image (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits) and catalog (wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat) found
'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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 163644 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.769457
a=0.000000 b=1.000000 c=22.769457
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 125 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
2.0 pix Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
2.4 pix fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
2.4 pix fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
Limiting magnitude estimates:
15.5 mag. Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
15.5 mag. Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
14.1 mag. fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
14.1 mag. fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.6 (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.rpC44dR1EI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=55, blended=21410, passed=163589
Got 163589 stars (including 141908 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 163589 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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.BYePc82TiC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=54, blended=21418, passed=163772
Got 163772 stars (including 142086 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 163772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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: 0.47"
Estimated accuracy of the plate solution: 0.49"
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_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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.4chFXe6ow7 (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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=3900, passed=62442
Got 62442 stars (including 58453 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 62442 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.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.I3FEe20NlB (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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3792, passed=60251
Got 60251 stars (including 56378 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat
util/solve_plate_with_UCAC5 got 60251 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.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-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/wcs_Tau-04-Q2b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Saving fully-calibrated image wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/wcs_Tau-04-Q2b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-42_20.00sec_-10.00C_LIGHT_0054.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.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_2026-03-29_CI_Tau-04-Q2b1x1_214301_TTUQ2b1x1_28049_Ho3Y7bFd/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055.fits
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out186199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194623.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out192799.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out188061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out188118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out198139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29777.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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: 4s
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Considering the candidate 186193_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186193_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:49:59.76 +20:35:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186199_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186199_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:49:27.28 +25:26:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.211 3428989708880200960 087.36367865011 +25.44727969999 13.7311 13.2620 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.211#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186206_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186206_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:56:05.03 +21:44:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186214_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186214_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:33.52 +17:55:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.986 3398095008388473728 086.88988880059 +17.91996450633 13.3156 12.9661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186216_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186216_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:34:49.06 +18:33:08.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)
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Considering the candidate 186221_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186221_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:53:37.88 +24:42:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186224_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186224_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:38:34.36 +21:42:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186225_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186225_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:57:09.95 +25:14:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.271 3428083608219422976 089.29171806937 +25.24943018380 13.2536 12.7347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186226_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186226_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:57:27.21 +23:49:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.295 3424841904341512320 089.36331097182 +23.82644629518 13.4470 12.9069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186230_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186230_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:44:57.13 +21:51:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.478 3403246671339006336 086.23769507651 +21.86610583183 12.2367 10.9640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186232_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186232_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:44:21.18 +18:32:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186236_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186236_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:40:37.43 +19:45:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186239_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186239_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:48:27.25 +20:47:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186241_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186241_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:50:04.20 +24:54:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186242_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186242_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:51:04.93 +22:35:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.510 3427284057106243072 087.77050087061 +22.58780793535 11.8600 10.9289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186246_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186246_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:49.00 +20:33:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186248_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 186248_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:38:22.98 +22:40:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 187233_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 187233_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:09:43.03 +23:02:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188061_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
Preparing report for the candidate 188061_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
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Considering the candidate 188118_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
Preparing report for the candidate 188118_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
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Considering the candidate 188874_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 188874_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:41:56.12 +22:38:55.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 189236_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 189236_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:58:01.83 +25:55:16.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 189842_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 189842_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:37:03.69 +20:44:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190421_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 190421_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:48:36.00 +23:46:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190570_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 190570_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:30:50.69 +22:27:24.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190702_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 190702_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:43:00.27 +18:59:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190833_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 190833_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:45:12.72 +18:24:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190844_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 190844_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:45:44.88 +23:44:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191013_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
Preparing report for the candidate 191013_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
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Considering the candidate 191327_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 191327_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:45:36.92 +25:05:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191336_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 191336_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:41:08.62 +21:18:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191359_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 191359_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:37:00.61 +20:46:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191452_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 191452_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:31:40.08 +18:13:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191522_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 191522_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:57:55.93 +24:36:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.518 3427997880672739072 089.48272794596 +24.61172721093 12.7050 11.9046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191659_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 191659_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:51:30.86 +18:25:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191730_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 191730_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:39:54.77 +23:40:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191761_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 191761_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:45:50.21 +21:18:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191886_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 191886_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:32:09.85 +18:33:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192037_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 192037_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:43:08.95 +20:03:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.390 3399548871998739200 085.78691270572 +20.06476701627 12.8658 12.5188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192062_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 192062_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:20:11.69 +19:34:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192478_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 192478_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:42:11.79 +22:40:39.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192559_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 192559_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:34:54.63 +19:28:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192692_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 192692_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:13.62 +21:51:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192799_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 192799_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:40:12.81 +24:31:54.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 192811_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 192811_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:48:06.79 +21:33:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192923_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 192923_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:51:02.22 +20:08:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193060_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193060_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:33:38.39 +18:33:24.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193072_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193072_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:58:48.25 +25:47:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193109_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193109_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:31:10.92 +20:10:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193123_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193123_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:39:37.25 +18:52:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193135_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193135_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:39:11.37 +19:48:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193148_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193148_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:02.92 +20:17:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193308_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193308_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:32.65 +23:52:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193428_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
Preparing report for the candidate 193428_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
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Considering the candidate 193453_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193453_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:18.61 +17:43:38.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193480_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193480_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:11:14.73 +23:03:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 5.030 3415724204168139392 077.81283494550 +23.05225482933 12.9099 12.5397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193561_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193561_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:46:40.13 +20:11:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193711_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193711_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:50:03.90 +19:09:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193729_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193729_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:44:42.24 +23:00:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193762_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193762_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:45:52.29 +21:18:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193793_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193793_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:44:21.82 +21:11:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193849_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193849_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:42:01.38 +19:41:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193870_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193870_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:32:02.88 +18:33:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193923_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193923_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:44:04.02 +24:38:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193939_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 193939_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:49:59.74 +22:34:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194062_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194062_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:29:17.11 +18:20:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194073_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194073_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:34:54.80 +22:33:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194239_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194239_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:43:37.21 +25:25:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194247_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194247_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:33:36.15 +18:33:24.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194277_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194277_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:45:11.22 +18:40:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194343_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194343_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:29.12 +18:44:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194346_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194346_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:35:28.97 +21:16:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194365_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
Preparing report for the candidate 194365_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
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Considering the candidate 194412_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194412_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:35:02.32 +24:18:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194529_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194529_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:35:18.96 +21:12:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194555_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194555_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:55:40.41 +20:26:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194567_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194567_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:49:49.40 +18:34:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194602_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194602_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:50:02.28 +22:58:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194611_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194611_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:43:53.37 +21:56:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194622_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194622_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:58:38.19 +20:44:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194623_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194623_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:58.78 +24:22:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 1.000 3427792508219215744 086.99491970101 +24.37138890811 13.5291 13.0457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194640_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194640_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:45:46.88 +22:42:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.230 3427521139301335680 086.44443127298 +22.70683543724 13.2578 12.2450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194700_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 194700_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:51:40.29 +23:12:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195049_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195049_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:30:36.68 +22:27:33.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 195088_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195088_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:36:07.77 +19:32:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195102_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195102_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:16:46.54 +20:08:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195194_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195194_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:05.65 +23:11:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195227_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195227_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:46:50.96 +20:15:56.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195376_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195376_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:28:32.15 +22:45:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195392_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195392_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:39:57.93 +24:13:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195404_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195404_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:41:10.63 +20:05:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195476_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195476_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:42:25.02 +18:03:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.398 3397587691149687040 085.60435118827 +18.06647309680 13.4200 13.0479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195561_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195561_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:48:54.90 +19:05:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195570_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195570_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:44:13.60 +25:22:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195596_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195596_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:39:27.42 +21:47:33.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195806_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195806_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:15:08.53 +20:02:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195945_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195945_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:20:15.07 +19:35:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195976_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 195976_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:52:10.89 +22:50:12.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196394_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 196394_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:42:18.21 +18:55:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.016 3399178890633638912 085.57600342173 +18.91764373490 12.6440 11.3777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196514_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 196514_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:48:17.29 +20:45:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196571_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 196571_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:47:48.31 +19:03:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196789_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 196789_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:40:30.85 +21:44:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 0.405 3403328752456864384 085.12842278463 +21.73571617574 13.2183 12.2378 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.405#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196895_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 196895_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:46:11.43 +25:40:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197084_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 197084_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:35:45.58 +21:24:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 0.875 3402983647541750144 083.94010905980 +21.40952997539 13.5901 13.0758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197131_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 197131_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:41:02.33 +24:22:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197315_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 197315_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:49:40.10 +23:42:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.856 3427677510470920832 087.41704882692 +23.70268023145 13.5544 12.9524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197469_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 197469_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:42:31.33 +18:39:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.418 3399117902098101376 085.63148935225 +18.65802480270 13.7753 13.1914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197750_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 197750_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:28:41.01 +18:57:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.304 3401066855176541696 082.17132693397 +18.95396798356 13.8343 13.2307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197766_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 197766_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 197803_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 197803_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:19:43.91 +26:10:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197963_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 197963_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:41:04.22 +20:48:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198062_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 198062_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:37:08.27 +22:06:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198139_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
Preparing report for the candidate 198139_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
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Considering the candidate 198331_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 198331_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:45:47.95 +21:18:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198449_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 198449_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:38:09.51 +18:34:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.958 3397841059859335424 084.54016242734 +18.57480141957 13.8510 12.8994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198699_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 198699_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 55654_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 55654_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:55:48.78 +20:10:33.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 56342_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 56342_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:16:29.02 +20:02:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79840_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 79840_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:53:50.48 +21:45:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62296_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 62296_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:32:32.95 +20:37:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18025_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 18025_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:46:56.43 +17:54:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89732_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 89732_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:08:17.10 +21:56:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131291_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 131291_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks
**** FOUND 05:30:04.39 +25:01:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132765_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055
The candidate 132765_fd_Tau-04-Q2b1x1_2026-03-29_21-40-35_20.00sec_-10.00C_LIGHT_0055 did not pass the final checks