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_214103_TTUQ2b1x1_21479_AUHOUj8J
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 30.1104* 05 52 12.86 +23 17 07.7 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 3427434793278648704,2461129.6104,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3427434793278648704 20260330.1104 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:12.86 +23:17:07.7 ;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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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 30.1104* 05 35 58.46 +24 44 53.3 9.6 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
CQ Tau,2461129.6104,9.60,0.05,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
CQ Tau 20260330.1104 9.60CV 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/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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:58.46 +24:44:53.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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 30.1104* 05 21 45.70 +20 54 41.3 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,2461129.6104,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1104 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:45.70 +20:54:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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 30.1104* 05 15 12.77 +25 58 00.0 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,2461129.6104,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1104 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:12.77 +25:58:00.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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 30.1104* 05 17 47.09 +18 30 02.0 12.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461129.6104,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1104 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:47.09 +18:30:02.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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 30.1104* 05 15 26.48 +22 06 50.4 12.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461129.6104,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1104 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:26.48 +22:06:50.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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 30.1104* 05 27 43.04 +19 11 47.5 13.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461129.6104,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1104 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:43.04 +19:11:47.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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 30.1104* 05 18 00.45 +18 21 18.1 11.6 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J051800+1821.3,2461129.6104,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J051800+1821.3 20260330.1104 11.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:00.45 +18:21:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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_21-39-11_20_00sec_-10_00C_LIGHT_0053_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_21-38-23_20_00sec_-9_90C_LIGHT_0052_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: 2461129.61066475 30.03.2026 02:39:11.434 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
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): 18621
Objects passed selection criteria: 18542
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: 13113.5
Average stars matched: 12282.5 (93.663 %)
Memory usage VmPeak: 123516 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 21:43:17 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: 2461129.61066475 30.03.2026 02:39:11.434 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 147
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: 29 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): 134995
Objects passed selection criteria: 134669
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: 97551.5
Average stars matched: 91019.8 (93.3043 %)
Memory usage VmPeak: 2093292 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 21:45:35 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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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: 2461129.61011215
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_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits'
wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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 05:32:18.750 +22:00:27.11
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:18.823 +22:00:58.28
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:32:18.750 +22:00:27.11
Second-epoch second image center 05:32:18.823 +22:00:58.28
Angular distance between the image centers 0.00866 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.tLpmkM0HhE
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.hloVQsBLXm
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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits &> /tmp/tmp.twNFjKntpX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits &> /tmp/tmp.FTfswwUKnx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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 4 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_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
2.5 pix fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
14.1 mag. fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
All-image limiting magnitude estimate: 14.1 (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.tLpmkM0HhE (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_214103_TTUQ2b1x1_21479_AUHOUj8J/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.hloVQsBLXm (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_214103_TTUQ2b1x1_21479_AUHOUj8J/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.twNFjKntpX (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_214103_TTUQ2b1x1_21479_AUHOUj8J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=676, passed=9077
Got 9077 stars (including 8393 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 9077 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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 931 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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.FTfswwUKnx (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_214103_TTUQ2b1x1_21479_AUHOUj8J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=618, passed=8945
Got 8945 stars (including 8315 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 8945 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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/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_214103_TTUQ2b1x1_21479_AUHOUj8J/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_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits'
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out18021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33090.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32140_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 32140_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:09:43.14 +23:02:03.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33090_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
Preparing report for the candidate 33090_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07693_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 07693_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:55:48.79 +20:10:33.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18021_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
Preparing report for the candidate 18021_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Tau-04-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 ####
05:35:58.46 +24:44:53.3
05:52:12.86 +23:17:07.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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 05:32:18.750 +22:00:27.11
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:18.823 +22:00:58.28
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:32:18.750 +22:00:27.11
Second-epoch second image center 05:32:18.823 +22:00:58.28
Angular distance between the image centers 0.00866 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.2Mh2ST3ZuH
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.NvD9OLsKUM
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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits &> /tmp/tmp.agdwLhitLD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits &> /tmp/tmp.sDHAtQj6yE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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 129 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_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
2.4 pix fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
14.1 mag. fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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.2Mh2ST3ZuH (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_214103_TTUQ2b1x1_21479_AUHOUj8J/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.NvD9OLsKUM (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_214103_TTUQ2b1x1_21479_AUHOUj8J/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.agdwLhitLD (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_214103_TTUQ2b1x1_21479_AUHOUj8J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=4165, passed=63909
Got 63909 stars (including 59641 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 63909 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 930 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: 0.64"
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 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.71"
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_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.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.sDHAtQj6yE (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_214103_TTUQ2b1x1_21479_AUHOUj8J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Tau-04-Q2b1x1_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=3925, passed=62077
Got 62077 stars (including 58062 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 62077 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: 0.64"
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 928 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_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits -region wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/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_214103_TTUQ2b1x1_21479_AUHOUj8J/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_21-38-23_20.00sec_-9.90C_LIGHT_0052.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_214103_TTUQ2b1x1_21479_AUHOUj8J/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-38-23_20.00sec_-9.90C_LIGHT_0052.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.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_214103_TTUQ2b1x1_21479_AUHOUj8J/wcs_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053.fits
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out186190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192509.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out193992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195692.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out195897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out196462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out188006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197249.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): 11s
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: 3s
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Considering the candidate 186190_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186190_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:14:31.18 +20:35:06.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
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Considering the candidate 186193_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186193_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:56:05.03 +21:44:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.342 3424026302935656704 089.02095141528 +21.74428937175 13.2832 12.3029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186198_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186198_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:41:59.92 +22:11:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186199_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186199_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:38:28.26 +18:08:57.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 186201_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186201_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:40:23.44 +18:17:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186205_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186205_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:53:37.93 +24:42:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.398 3428135590204488320 088.40825642168 +24.71447472774 12.6638 11.4645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186209_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186209_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:36:28.60 +19:17:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 3.055 3400959236178459904 084.11961886311 +19.28812237404 13.3975 12.7870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186212_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186212_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:42:01.43 +19:41:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.744 3399439195713252480 085.50516345102 +19.69531157119 13.2929 12.7613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186213_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186213_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:44:21.16 +18:32:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186215_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186215_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:48:40.18 +18:57:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 0.651 3398495715955368448 087.16741377275 +18.96123632260 12.9678 12.4962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.651#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_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186216_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:34:30.77 +19:49:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186221_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186221_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:40:37.42 +19:45:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186223_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186223_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:49:30.56 +19:19:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.573 3398886588042948352 087.37689177674 +19.32324721114 12.8416 12.3708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186225_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186225_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:35:58.13 +24:15:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186227_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186227_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:50:04.12 +24:54:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.363 3428189122677094656 087.51748553604 +24.91336658141 12.3228 11.4765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186228_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186228_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:48:27.34 +20:47:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 1.063 3399984519120424704 087.11362136452 +20.79824337407 12.3659 11.6799 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186229_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186229_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:51:06.42 +22:35:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186232_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186232_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:58:11.94 +21:57:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.798 3424057398497650176 089.54955142398 +21.96154323215 12.0764 11.5777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186234_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186234_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:47:48.99 +20:33:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186235_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 186235_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:22:27.41 +19:14:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 0.635 3401509992722123904 080.61429630533 +19.23640557468 10.9805 10.1520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187231_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 187231_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:09:43.08 +23:02:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188006_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
Preparing report for the candidate 188006_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
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Considering the candidate 188150_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 188150_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:52:12.89 +23:17:08.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 188694_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 188694_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:41:56.17 +22:38:55.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 189266_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 189266_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:58:01.81 +25:55:16.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 189611_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 189611_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:37:03.72 +20:44:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 1.546 3402798512973317760 084.26595723537 +20.74448566277 11.6391 10.5576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189964_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 189964_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:46:35.68 +25:17:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 1.776 3429021246820626944 086.64913731373 +25.28424955093 12.3632 11.8441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190549_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 190549_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:48:35.95 +23:46:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 2.021 3427689914336506368 087.15038315123 +23.77049007997 11.5312 10.2792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190550_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 190550_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:45:12.72 +18:24:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.490 3398370848369487616 086.30342774195 +18.40469599223 12.3881 11.5910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190596_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 190596_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:30:50.66 +22:27:24.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 190635_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 190635_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:41:08.60 +21:18:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190765_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 190765_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:45:44.91 +23:44:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.079 3427654317646750464 086.43686085122 +23.74257266285 12.7173 12.3944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191083_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
Preparing report for the candidate 191083_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
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Considering the candidate 191300_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 191300_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:43:00.29 +18:59:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191340_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 191340_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:37:00.60 +20:46:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.083 3402799170106624512 084.25261155847 +20.77964331919 12.4805 11.5406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191378_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 191378_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:32:09.88 +18:33:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.244 3400795791199970176 083.04105692218 +18.55319834212 12.3419 11.4984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191462_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 191462_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:31:40.03 +18:13:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.038 3400405597720683008 082.91707229208 +18.22052626417 12.4331 11.6071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191734_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 191734_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:45:50.22 +21:18:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191858_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 191858_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:45:36.95 +25:05:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191922_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 191922_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:51:30.81 +18:25:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191960_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 191960_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:42:46.98 +21:22:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192021_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192021_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:47:13.78 +21:51:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.323 3403213548551009792 086.80781257479 +21.86531159229 12.5663 11.6077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192054_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192054_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:39:37.33 +18:52:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192075_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192075_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:42:11.84 +22:40:39.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192197_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192197_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:58:40.27 +20:44:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.367 3423066944680520832 089.66770544496 +20.73868455323 12.6129 11.5579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192268_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192268_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:58:48.25 +25:47:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192319_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192319_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:33:38.38 +18:33:24.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192417_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192417_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:45:52.34 +21:18:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192490_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192490_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:47:02.94 +20:17:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192509_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192509_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:43:19.25 +20:18:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.242 3399626735462144384 085.82986908223 +20.31342183506 13.0548 12.5007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192511_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192511_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:20:11.75 +19:34:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192778_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
Preparing report for the candidate 192778_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
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Considering the candidate 192822_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192822_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:47:18.63 +17:43:37.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 192899_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192899_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:34:54.64 +19:28:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.932 3400979886382336768 083.72772804333 +19.47739469377 12.8834 12.4476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192931_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 192931_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:31:10.94 +20:10:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193084_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193084_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:29:17.11 +18:20:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193092_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193092_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:39:11.38 +19:48:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193111_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193111_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:44:21.86 +21:11:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193183_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193183_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:44:03.98 +24:38:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193217_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193217_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:51:02.19 +20:08:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193349_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
Preparing report for the candidate 193349_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
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Considering the candidate 193402_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193402_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:45:11.25 +18:40:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193419_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193419_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:44:42.23 +23:00:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193462_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193462_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:34:54.82 +22:33:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193465_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193465_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:49:28.74 +21:19:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.395 3400131445660143744 087.36974819773 +21.32322087589 13.1560 12.3148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 193559_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193559_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:58:38.26 +20:44:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193579_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193579_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:47:32.62 +23:52:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193662_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193662_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:32:02.94 +18:33:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193954_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193954_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:33:36.16 +18:33:24.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193992_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 193992_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:34:56.21 +20:14:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.768 3402753574733953408 083.73453670225 +20.24143798682 13.2174 12.4240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194007_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194007_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:49:59.71 +22:34:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.095 3427282300462335104 087.49911072441 +22.57650207800 12.8636 11.8742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194060_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194060_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:35:02.34 +24:18:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 4.164 3416698848209737344 083.75970265763 +24.31351700282 12.3204 11.1110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194177_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194177_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:50:02.30 +22:57:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.025 3427356453074603008 087.51003407546 +22.96701848032 13.1969 12.6712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194209_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194209_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:55:40.38 +20:26:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194248_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194248_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:46:40.15 +20:11:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194280_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194280_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:35:19.04 +21:12:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194300_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194300_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:49:49.38 +18:34:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.634 3398401226675505152 087.45593541073 +18.57973333703 13.1643 12.6343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194323_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194323_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:28:32.27 +22:45:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194343_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194343_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:36:07.84 +19:32:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194374_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194374_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:50:03.86 +19:09:39.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)
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Considering the candidate 194424_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194424_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:48:54.91 +19:05:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194740_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194740_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:47:48.31 +19:03:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.096 3398512651009075712 086.95228042340 +19.06623256805 13.4256 12.6871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194830_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194830_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:51:40.20 +23:12:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.063 3427413662039588608 087.91869185340 +23.21486717539 13.6687 13.0826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194866_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 194866_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:39:58.04 +24:13:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195019_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195019_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:41:10.60 +20:05:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.214 3399605363704742656 085.29386315031 +20.08570769140 12.9727 12.0984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195027_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195027_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:46:50.94 +20:15:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195034_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195034_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:41:22.40 +23:21:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.964 3404355838052678400 085.34322390235 +23.35155372241 13.5645 13.0281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195087_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195087_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:36:29.27 +21:58:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.981 3403784744842342656 084.12224662201 +21.97719741463 13.2921 12.7133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195190_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195190_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:48:17.31 +20:45:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.594 3399983767504237184 087.07230090399 +20.75667869551 13.3908 12.9285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195318_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195318_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:52:25.69 +24:07:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195323_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195323_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:44:13.66 +25:22:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195578_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195578_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:53:40.18 +20:19:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195583_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195583_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:43:53.37 +21:56:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.055 3403261995781890176 085.97267317403 +21.93726443789 13.3584 12.9596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195686_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195686_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:44:28.77 +22:45:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.298 3403517975832657792 086.11949068234 +22.76596068508 13.5999 13.0715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195691_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195691_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:41:02.34 +24:22:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.217 3428662604170066816 085.25950498940 +24.37139278562 11.5971 9.9128 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195692_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195692_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:32:41.17 +20:56:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.851 3403604351917433472 083.17201916460 +20.93470015681 13.3470 12.9289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195783_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195783_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:37:09.19 +19:14:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.242 3397961525101590016 084.28796428920 +19.23556851358 13.4543 12.7942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195829_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195829_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:15:08.54 +20:02:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195897_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195897_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:19:10.29 +19:41:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 5.160 3401693748602381312 079.79433852135 +19.68588355623 13.4472 12.5854 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 195967_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195967_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:47:29.16 +18:44:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195972_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 195972_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:47:05.70 +23:11:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196139_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196139_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:54:01.56 +21:49:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196191_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196191_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:46:11.47 +25:41:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196196_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196196_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:43:37.06 +25:25:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196334_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196334_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:45:20.22 +24:24:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196356_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196356_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:18:29.64 +21:46:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196442_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196442_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:30:43.21 +17:55:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196462_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196462_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:49:31.67 +20:45:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.651 3399890102857495680 087.38267657704 +20.76158002105 13.6397 13.1455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 196844_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196844_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:51:00.25 +24:57:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196908_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196908_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:41:04.30 +20:48:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196917_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196917_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:16:46.39 +20:08:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196965_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 196965_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:19:44.04 +26:10:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197021_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 197021_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:44:41.90 +24:36:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197249_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
Preparing report for the candidate 197249_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
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Considering the candidate 197376_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 197376_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:41:52.50 +23:20:37.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197449_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 197449_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:41:07.08 +24:22:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197452_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 197452_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:35:34.58 +21:24:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197518_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 197518_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:43:10.29 +18:50:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197580_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 197580_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:36:21.88 +24:21:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197860_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 197860_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:45:37.96 +19:23:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198473_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 198473_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:47:53.26 +22:13:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56342_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 56342_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:16:29.04 +20:02:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55654_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 55654_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:55:48.77 +20:10:33.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 89732_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 89732_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:08:17.09 +21:56:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131291_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 131291_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:30:04.44 +25:01:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18025_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 18025_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:46:56.47 +17:54:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62296_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 62296_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks
**** FOUND 05:32:32.98 +20:37:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79840_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053
The candidate 79840_fd_Tau-04-Q2b1x1_2026-03-29_21-39-11_20.00sec_-10.00C_LIGHT_0053 did not pass the final checks