This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7
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,2461126.9292,11.79,0.05,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 20260327.4292 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:09:53.06 -14:57:37.0 ;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-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_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,2461126.9292,12.18,0.05,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 20260327.4292 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:20:26.18 -21:11:12.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_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,2461126.9292,12.35,0.05,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 20260327.4292 12.35CV 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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:58:37.35 -16:04:25.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_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,2461126.9292,13.07,0.05,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 20260327.4292 13.07CV 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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:22:37.09 -14:32:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_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
GI Lib,2461126.9292,12.06,0.05,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
GI Lib 20260327.4292 12.06CV 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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:04:41.85 -17:25:08.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20_00sec_-15_00C_LIGHT_0471_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20_00sec_-15_00C_LIGHT_0225_fits__*pix.png resample_wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20_00sec_-14_90C_LIGHT_0470_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: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461126.92952187 27.03.2026 10:18:20.690 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.28
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): 6784
Objects passed selection criteria: 6778
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 5814.75
Average stars matched: 5367.5 (92.3084 %)
Memory usage VmPeak: 112640 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 06:35:52 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: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461126.92952187 27.03.2026 10:18:20.690 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 168
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.97
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: 13 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): 42498
Objects passed selection criteria: 42424
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 37108.8
Average stars matched: 34311.8 (92.4627 %)
Memory usage VmPeak: 141144 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 06:36:41 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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.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: 2461126.92894660
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits'
wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:24.771 -18:01:29.97
Angular distance between the image centers 0.16 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 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:27.161 -18:02:04.18
Angular distance between the image centers 0.15 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 15:06:24.771 -18:01:29.97
Second-epoch second image center 15:06:27.161 -18:02:04.18
Angular distance between the image centers 0.01341 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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.P34dhAQUi9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.78XMUJ0TGi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits &> /tmp/tmp.nw8qCq8CHP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits &> /tmp/tmp.ZZtBFqUarP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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 4760 out of 6705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.861505
a=0.000000 b=1.000000 c=22.861505
From vast_summary.log: estimated ref. image limiting mag.: -8.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.4 pix Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
2.5 pix fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
2.7 pix fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
Limiting magnitude estimates:
14.6 mag. Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.6 mag. Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
14.5 mag. fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
14.6 mag. fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.P34dhAQUi9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=403, passed=6705
Got 6705 stars (including 6294 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 6705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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.78XMUJ0TGi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=425, passed=6649
Got 6649 stars (including 6218 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 6649 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 958 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.nw8qCq8CHP (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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=297, passed=6820
Got 6820 stars (including 6515 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat
util/solve_plate_with_UCAC5 got 6820 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits -region wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.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.ZZtBFqUarP (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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=306, passed=7143
Got 7143 stars (including 6833 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat
util/solve_plate_with_UCAC5 got 7143 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 959 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 959 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: 0.42"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits -region wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
Saving fully-calibrated image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits'
Preparing the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out21058.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20274_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 20274_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:17:57.87 -13:57:48.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21044_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 21044_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:13:58.26 -13:58:52.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21058_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
Preparing report for the candidate 21058_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01970_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 01970_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:42:46.42 -20:12:35.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Lib-03-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 ####
15:09:53.06 -14:57:37.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits exists and is non-empty
wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:24.771 -18:01:29.97
Angular distance between the image centers 0.16 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 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:27.161 -18:02:04.18
Angular distance between the image centers 0.15 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 15:06:24.771 -18:01:29.97
Second-epoch second image center 15:06:27.161 -18:02:04.18
Angular distance between the image centers 0.01341 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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.BdAcIxp3Vw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.rdr9lUChfk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits &> /tmp/tmp.tIsiB4YRSl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits &> /tmp/tmp.iJYE1JKjsp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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 5340 out of 42407 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.687465
a=0.000000 b=1.000000 c=22.687465
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.72
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.72
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 67 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.3 pix Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
2.5 pix fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
2.6 pix fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
Limiting magnitude estimates:
14.7 mag. Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.7 mag. Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
14.6 mag. fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
14.6 mag. fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BdAcIxp3Vw (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1940, passed=42401
Got 42401 stars (including 40414 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 42401 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 955 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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.rdr9lUChfk (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1927, passed=42823
Got 42823 stars (including 40848 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 42823 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 958 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.tIsiB4YRSl (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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1523, passed=40189
Got 40189 stars (including 38613 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat
util/solve_plate_with_UCAC5 got 40189 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits -region wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.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.iJYE1JKjsp (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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1733, passed=41040
Got 41040 stars (including 39257 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat
util/solve_plate_with_UCAC5 got 41040 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 955 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: 0.41"
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 955 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: 0.41"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits -region wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.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-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Saving fully-calibrated image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-17-30_20.00sec_-14.90C_LIGHT_0470.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.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_2026-03-27_CI_Lib-03-Q2b1x1_063342_TTUQ2b1x1_13205_MkWJakZ7/wcs_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471.fits
Preparing the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58281.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58532.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out58984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out23565.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55534.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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 53266_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 53266_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:31:15.04 -19:47:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53270_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 53270_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:29:24.42 -19:46:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.417 6254491531477367296 232.35181373509 -19.76927794963 14.0320 13.3735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53279_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 53279_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:16:05.06 -18:06:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.290 6257381975743519488 229.02099843925 -18.10177779418 13.3260 12.4771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53282_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 53282_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:32:08.06 -14:52:33.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 53284_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 53284_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:29:29.59 -18:23:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54057_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 54057_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:09:53.06 -14:57:37.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 54440_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
Preparing report for the candidate 54440_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
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Considering the candidate 54611_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
Preparing report for the candidate 54611_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
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Considering the candidate 55406_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 55406_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:30:20.55 -15:37:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55534_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
Preparing report for the candidate 55534_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
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Considering the candidate 56340_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 56340_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:32:49.31 -19:36:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56448_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 56448_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:29:50.07 -19:50:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56726_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 56726_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:22:53.44 -22:05:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57586_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 57586_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:57:02.86 -16:18:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57695_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 57695_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:25:49.91 -22:04:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57707_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 57707_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:25:35.84 -22:02:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57734_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 57734_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:24:18.78 -21:26:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57757_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 57757_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:24:46.05 -21:39:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57808_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 57808_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:25:46.21 -21:25:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58057_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58057_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:32:10.10 -18:32:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58076_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58076_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:13:35.38 -19:04:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.937 6256474839996977280 228.39767346928 -19.06867461510 14.3597 13.7660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58108_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58108_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:31:38.34 -16:48:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 2.768 6258516912267678336 232.90901940358 -16.80445855818 14.1787 13.6200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58173_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58173_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:29:11.17 -19:04:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58253_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58253_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:21:54.35 -22:04:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58260_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58260_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:32:27.94 -19:14:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.861 6254583753015355776 233.11596145431 -19.23998156392 14.1028 13.5766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58271_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58271_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:31:25.33 -19:50:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58280_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58280_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:29:35.51 -18:25:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58281_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58281_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:18:34.27 -21:35:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.301 6252582092096494464 229.64275731398 -21.58472100225 13.8496 13.1013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58325_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58325_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:18:09.93 -21:52:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.888 6252364766753755008 229.54135666108 -21.87096830175 14.0144 13.7127 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58351_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58351_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:24:14.32 -22:02:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58366_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58366_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:31:48.42 -14:41:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.998 6265790181680012160 232.95172624530 -14.68630713005 13.9170 13.1227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58370_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58370_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:25:00.95 -22:14:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58379_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58379_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:06:07.65 -21:19:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58405_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58405_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:32:07.87 -14:20:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.594 6265840312538423680 233.03263976925 -14.33588972266 14.1155 13.3567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58406_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58406_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:32:46.02 -19:34:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.198 6254554203640411904 233.19139741944 -19.57368509694 14.0372 13.5060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58408_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58408_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:49:02.10 -18:50:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.792 6282016946080033152 222.25886549479 -18.84820796891 14.3886 13.8904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58417_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58417_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:23:16.19 -21:25:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.500 6252739768937524352 230.81723014546 -21.42338627889 13.9168 13.2312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 58418_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58418_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:32:14.38 -18:43:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58463_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58463_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:31:39.84 -19:05:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58532_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58532_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:25:41.09 -13:50:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 0.345 6266149309664155136 231.42125800526 -13.83399934876 14.2869 13.6531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58632_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58632_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:47:24.93 -21:33:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58645_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58645_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:18:57.00 -22:13:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.462 6252289072250033664 229.73758891092 -22.22165406880 14.0133 13.4631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58659_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58659_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:06:05.13 -21:21:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.497 6231773456579126784 226.52107926506 -21.36308921096 14.3372 13.6207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58677_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58677_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:31:56.01 -14:02:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.410 6266271080580723456 232.98299848912 -14.04500233192 14.2431 13.6616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58684_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58684_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:19:22.84 -22:13:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.034 6252293916973305728 229.84541042421 -22.21940002450 14.0702 13.4135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58690_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58690_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:21:13.01 -18:09:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 1.564 6258095352631494656 230.30375116927 -18.15697473351 14.4045 13.8303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58708_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58708_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:26:02.00 -21:03:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.607 6252838312666027392 231.50793490697 -21.06089162873 14.0098 13.4842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58712_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58712_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:20:10.07 -21:12:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58734_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58734_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:14:25.71 -19:13:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58740_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58740_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:21:35.14 -19:10:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.695 6257774295237419776 230.39575864586 -19.16816712505 14.3245 13.8069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58744_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58744_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:01:37.65 -21:32:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.296 6232457627689515648 225.40681031679 -21.54888940672 14.3392 13.7823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58769_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58769_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:30:50.83 -17:23:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58776_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58776_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:00:07.57 -21:10:25.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.238 6232531260608816640 225.03153912835 -21.17335066717 14.1711 13.4867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58832_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58832_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:20:43.91 -19:18:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.302 6256271194121805184 230.18287088285 -19.30037553940 14.0677 13.4396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58841_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58841_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:52:20.02 -22:03:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.174 6232192129990856960 223.08339959865 -22.05925975686 14.2740 13.6902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58850_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58850_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:23:06.84 -19:34:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 0.735 6254743800678381056 230.77869983402 -19.57502347280 14.2438 13.6011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58858_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58858_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:47:38.11 -16:22:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.178 6309626954363605376 221.90846150476 -16.37383211876 14.2702 13.6930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58863_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58863_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:22:58.18 -21:38:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.297 6252701698347241600 230.74234181942 -21.64695191775 14.0602 13.4622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58872_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58872_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:50:05.01 -21:41:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58893_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58893_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:01:11.73 -22:12:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 0.612 6231649898959733632 225.29871762345 -22.20817100378 14.1382 13.4717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58920_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58920_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 15:11:53.56 -20:55:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.892 6255622963297313152 227.97379059282 -20.92610854585 14.2885 13.6338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58926_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58926_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:54:31.88 -21:03:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.425 6232398357140737536 223.63312502429 -21.06535160630 14.2148 13.6545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.425#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58946_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58946_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:50:10.43 -16:14:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.863 6309606304160944896 222.54370548195 -16.24582677146 14.3419 13.6698 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58984_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 58984_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:48:51.57 -22:01:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 0.320 6232231231373036544 222.21491406958 -22.02013678091 14.1881 13.6685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59021_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 59021_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks
**** FOUND 14:50:33.42 -21:40:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10485_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471
The candidate 10485_fd_Lib-03-Q2b1x1_2026-03-27_05-18-20_20.00sec_-15.00C_LIGHT_0471 did not pass the final checks