This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461119.8115,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.3115 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:43:26.08 -11:34:01.0 ;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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.8115,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.3115 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:27:32.56 -11:32:58.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.8115,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.3115 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:57:42.44 -11:48:25.5 ;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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.8115,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.3115 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:23:18.37 -09:11:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_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 20.3116* 14 30 06.38 -07 29 45.4 14.1 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461119.8115,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.3115 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:30:06.38 -07:29:45.4 ;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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20_00sec_-15_00C_LIGHT_0344_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20_00sec_-14_90C_LIGHT_0033_fits__*pix.png resample_wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20_00sec_-15_00C_LIGHT_0343_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: 2461059.01791420 18.01.2026 12:25:37.787 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
First image: 2461059.01791420 18.01.2026 12:25:37.787 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Last image: 2461119.81181683 20.03.2026 07:28:50.974 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.83
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5535
Objects passed selection criteria: 5535
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 5322.5
Average stars matched: 5209 (97.8675 %)
Memory usage VmPeak: 112052 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 02:38:01 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: 2461059.01791420 18.01.2026 12:25:37.787 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
First image: 2461059.01791420 18.01.2026 12:25:37.787 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Last image: 2461119.81181683 20.03.2026 07:28:50.974 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 328
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 12 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): 37505
Objects passed selection criteria: 37403
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 35345.2
Average stars matched: 34177.2 (96.6955 %)
Memory usage VmPeak: 140544 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 02:38:42 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/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.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/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.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: 2461119.81127637
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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits exists and is non-empty
Saving wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits to local_wcs_cache/
'wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits'
wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits exists and is non-empty
Saving wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits to local_wcs_cache/
'wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits' -> 'local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits'
wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits'
wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits exists and is non-empty
Saving wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits to local_wcs_cache/
'wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits' -> 'local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.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 14:34:18.609 -09:59:52.98
Second-epoch image center 14:34:30.526 -10:01:11.05
Angular distance between the image centers 0.05 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 14:34:18.609 -09:59:52.98
Second-epoch image center 14:34:31.857 -10:01:04.79
Angular distance between the image centers 0.06 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 14:34:30.526 -10:01:11.05
Second-epoch second image center 14:34:31.857 -10:01:04.79
Angular distance between the image centers 0.00573 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/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits &> /tmp/tmp.gh5iW1c9YR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits &> /tmp/tmp.wqHxnLcpaq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits &> /tmp/tmp.bdZz0mZIXX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits &> /tmp/tmp.PIa83GP7ep
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
Found non-empty wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
The reference image (wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits) and catalog (wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat) found
'wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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 3807 out of 6729 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.871094
a=0.000000 b=1.000000 c=22.871094
From vast_summary.log: estimated ref. image limiting mag.: -7.83
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
2.1 pix Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
2.5 pix fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
2.5 pix fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
Limiting magnitude estimates:
15.0 mag. Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
15.0 mag. Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
14.8 mag. fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
14.8 mag. fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gh5iW1c9YR (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/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits' -> 'wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=516, passed=6729
Got 6729 stars (including 6204 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 6729 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits -region wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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.wqHxnLcpaq (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/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits' -> 'wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=536, passed=6698
Got 6698 stars (including 6151 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
util/solve_plate_with_UCAC5 got 6698 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits -region wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.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.bdZz0mZIXX (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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=416, passed=6405
Got 6405 stars (including 5986 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat
util/solve_plate_with_UCAC5 got 6405 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits -region wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.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.PIa83GP7ep (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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=405, passed=6424
Got 6424 stars (including 6016 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat
util/solve_plate_with_UCAC5 got 6424 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits -region wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits'
Saving fully-calibrated image wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits'
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits'
Preparing the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20248_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 20248_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:46:18.37 -07:15:50.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20268_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 20268_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:10:21.57 -13:18:13.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20290_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 20290_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:36:20.04 -10:31:03.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat to cache
SExtractor catalog cache: saved Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Creating symlink local_wcs_cache/wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits exists and is non-empty
wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits exists and is non-empty
wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits exists and is non-empty
wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.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 14:34:18.609 -09:59:52.98
Second-epoch image center 14:34:30.526 -10:01:11.05
Angular distance between the image centers 0.05 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 14:34:18.609 -09:59:52.98
Second-epoch image center 14:34:31.857 -10:01:04.79
Angular distance between the image centers 0.06 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 14:34:30.526 -10:01:11.05
Second-epoch second image center 14:34:31.857 -10:01:04.79
Angular distance between the image centers 0.00573 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/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits &> /tmp/tmp.edkYI2CwMA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits &> /tmp/tmp.rHBdDYEB9j
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits &> /tmp/tmp.3BYA7JfkEe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits &> /tmp/tmp.GKnxYrnbTo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
Found non-empty wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits and wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
The reference image (wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits) and catalog (wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat) found
'wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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 3945 out of 44688 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.729906
a=0.000000 b=1.000000 c=22.729906
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 159 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
1.9 pix Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
2.3 pix fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
2.3 pix fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
Limiting magnitude estimates:
15.2 mag. Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
15.2 mag. Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
15.0 mag. fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
15.0 mag. fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.edkYI2CwMA (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/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits' -> 'wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1825, passed=44675
Got 44675 stars (including 42782 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 44675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 971 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits -region wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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.rHBdDYEB9j (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/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits' -> 'wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS_IMAGE_NAME=wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS-calibrated image found: wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Checking if the catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits alredy exist and is non-empty...
Catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat corresponding to the image wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
WCS catalog name: wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1859, passed=44694
Got 44694 stars (including 42756 good ones) from the SExtractor catalog wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat
util/solve_plate_with_UCAC5 got 44694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits -region wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.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.3BYA7JfkEe (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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1620, passed=37372
Got 37372 stars (including 35710 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat
util/solve_plate_with_UCAC5 got 37372 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits -region wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.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.GKnxYrnbTo (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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
WCS_IMAGE_NAME=wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
WCS-calibrated image found: wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
Checking if the catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
WCS catalog name: wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1581, passed=37244
Got 37244 stars (including 35616 good ones) from the SExtractor catalog wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat
util/solve_plate_with_UCAC5 got 37244 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits -region wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.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_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/wcs_Lib-01-Q2b1x1_2026-01-18_06-25-37_20.00sec_-14.90C_LIGHT_0033.fits
Saving fully-calibrated image wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/wcs_Lib-01-Q2b1x1_2026-01-18_06-26-20_20.00sec_-15.00C_LIGHT_0034.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-04_20.00sec_-15.00C_LIGHT_0343.fits
Saving fully-calibrated image wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.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_2026-03-20_CI_Lib-01-Q2b1x1_023551_TTUQ2b1x1_32053_9XimuIRX/wcs_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344.fits
Preparing the HTML report for the field Lib-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53468.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 53065_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53065_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:20:33.76 -10:18:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.162 6328716675244787840 215.14131383325 -10.31092255941 14.6510 13.7970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53067_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53067_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:37:49.88 -08:52:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.329 6329917341942564224 219.45753775599 -08.87333671430 14.8082 14.2528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53071_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53071_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:56:40.75 -08:27:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 0.883 6332422682265422848 224.16956707982 -08.45474295117 14.1297 13.4996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53073_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53073_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:53:05.29 -06:12:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.353 6336741426500492544 223.27212816393 -06.21275870098 14.7607 14.2546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53080_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53080_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:12:01.00 -05:53:40.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.311 3640985892993072128 213.00401756596 -05.89497149299 13.0373 12.5325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53081_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53081_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:29:27.77 -12:05:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.118 6324518460676133632 217.36566171574 -12.08927616237 12.7958 12.0016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53107_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53107_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 53125_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53125_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 53129_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
Preparing report for the candidate 53129_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
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Considering the candidate 53142_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53142_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 53143_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53143_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 53158_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53158_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 53161_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53161_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 53167_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53167_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 53171_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53171_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 53174_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53174_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
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Considering the candidate 53176_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53176_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 53177_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53177_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 53184_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53184_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 53194_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53194_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 53195_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53195_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53196_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53196_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 53198_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53198_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53199_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53199_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 53205_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53205_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 53206_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53206_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 53207_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53207_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 53209_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53209_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 53211_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53211_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 53215_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53215_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:52:03.24 -07:22:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53217_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53217_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 53223_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53223_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53225_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53225_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 53227_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53227_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 53232_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53232_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 53238_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53238_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 53246_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53246_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 53248_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53248_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 53266_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53266_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
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Considering the candidate 53267_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53267_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 53274_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53274_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 53278_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53278_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
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Considering the candidate 53279_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53279_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53283_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53283_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53286_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53286_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53287_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53287_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53294_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53294_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53297_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53297_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53299_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53299_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53300_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53300_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53301_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53301_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:07:04.05 -08:25:46.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53308_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53308_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53310_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53310_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53311_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53311_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53312_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53312_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53314_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53314_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53315_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53315_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:56:14.13 -05:56:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.552 6334116754806083072 224.05852937838 -05.94634367746 13.7343 13.0235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53316_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53316_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53318_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53318_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53319_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53319_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53321_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53321_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53325_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53325_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53329_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53329_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53331_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53331_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (19.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53336_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53336_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53337_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53337_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53338_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53338_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53340_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53340_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53341_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53341_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53347_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53347_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53349_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53349_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53357_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53357_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53359_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53359_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53360_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53360_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53361_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53361_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53363_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53363_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53364_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53364_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53366_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53366_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53370_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
Preparing report for the candidate 53370_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53372_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53372_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53377_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53377_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53378_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53378_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53381_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53381_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53387_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53387_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53390_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53390_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53394_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53394_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53397_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53397_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53398_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53398_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53405_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53405_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53407_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53407_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53409_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
Preparing report for the candidate 53409_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53412_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53412_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53414_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53414_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53417_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
Preparing report for the candidate 53417_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53420_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53420_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53424_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53424_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53425_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53425_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53426_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53426_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53428_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53428_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53435_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53435_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:47:38.36 -07:00:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.291 6330578663826723968 221.90952593428 -07.00266081813 14.8669 14.4453 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53437_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53437_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53439_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53439_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53441_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53441_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53442_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53442_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53443_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53443_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53448_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53448_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53452_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53452_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53454_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53454_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53456_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53456_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53457_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53457_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53459_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53459_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53461_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53461_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53462_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53462_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53463_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53463_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53466_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53466_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53467_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53467_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53468_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
Preparing report for the candidate 53468_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53469_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53469_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:22:18.31 -11:48:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 3.422 6303595411530667520 215.57726276424 -11.80740848047 14.1873 13.6307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53471_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53471_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53472_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53472_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53473_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53473_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53474_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53474_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53475_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53475_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53476_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53476_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53479_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53479_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53482_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53482_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53484_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53484_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53486_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53486_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53491_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53491_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53493_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53493_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53495_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53495_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53496_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53496_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53497_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53497_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53501_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53501_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53504_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53504_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53505_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53505_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53508_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53508_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53517_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53517_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53518_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53518_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53522_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53522_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53523_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53523_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53525_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53525_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53529_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53529_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53535_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53535_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53537_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53537_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53539_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53539_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53542_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53542_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53545_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53545_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53546_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53546_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53547_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53547_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53558_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53558_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53564_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53564_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53565_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53565_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53580_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53580_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:49:48.24 -06:32:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.095 6336621407934221056 222.45100466726 -06.54427956546 14.5581 14.0520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53584_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53584_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53587_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53587_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53597_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 53597_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
Rejecting candidate due to large distance (20.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07974_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 07974_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks
**** FOUND 14:10:21.61 -13:18:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39330_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344
The candidate 39330_fd_Lib-01-Q2b1x1_2026-03-20_02-28-50_20.00sec_-15.00C_LIGHT_0344 did not pass the final checks