This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A
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
NSVS J0419084+573821,2461129.6127,11.24,0.05,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
NSVS J0419084+573821 20260330.1127 11.24CV 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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:19:08.31 +57:38:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_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
Gaia DR3 445273145210225408,2461129.6127,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 445273145210225408 20260330.1127 12.99CV 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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:10.56 +55:30:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.1126* 03 37 09.26 +49 40 01.7 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0337086+493957,2461129.6127,12.99,0.05,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
NSVS J0337086+493957 20260330.1127 12.99CV 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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:09.26 +49:40:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.1126* 03 54 21.61 +51 28 39.5 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0354219+512839,2461129.6127,13.01,0.05,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
NSVS J0354219+512839 20260330.1127 13.01CV 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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:21.61 +51:28:39.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_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
GU Cam,2461129.6127,12.59,0.05,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
GU Cam 20260330.1127 12.59CV 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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:46.42 +55:55:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20_00sec_-10_00C_LIGHT_0057_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png resample_wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20_00sec_-10_00C_LIGHT_0056_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: 2461058.60610205 18.01.2026 02:32:37.217 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
First image: 2461058.60610205 18.01.2026 02:32:37.217 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
Last image: 2461129.61293928 30.03.2026 02:42:27.954 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 16243
Objects passed selection criteria: 16169
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 11306.2
Average stars matched: 10721.5 (94.8281 %)
Memory usage VmPeak: 121336 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 21:47:21 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: 2461058.60610205 18.01.2026 02:32:37.217 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
First image: 2461058.60610205 18.01.2026 02:32:37.217 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
Last image: 2461129.61293928 30.03.2026 02:42:27.954 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 86
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 30 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 119680
Objects passed selection criteria: 119373
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 86302.8
Average stars matched: 81003 (93.8591 %)
Memory usage VmPeak: 1885316 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 21:49:43 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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
SExtractor catalog cache: saved Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
SExtractor catalog cache: saved Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461129.61236350
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
Saving wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits to local_wcs_cache/
'wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits' -> 'local_wcs_cache/wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits'
wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits exists and is non-empty
Saving wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits to local_wcs_cache/
'wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits' -> 'local_wcs_cache/wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits'
wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits exists and is non-empty
Saving wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits to local_wcs_cache/
'wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits' -> 'local_wcs_cache/wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits'
wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits exists and is non-empty
Saving wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits to local_wcs_cache/
'wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits' -> 'local_wcs_cache/wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:14:05.422 +54:00:05.55
Second-epoch image center 04:14:06.659 +54:00:30.27
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:14:05.422 +54:00:05.55
Second-epoch image center 04:14:03.470 +54:00:43.50
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:14:06.659 +54:00:30.27
Second-epoch second image center 04:14:03.470 +54:00:43.50
Angular distance between the image centers 0.00863 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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.9sBGs61E8g
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits &> /tmp/tmp.MhjSrKfKTL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits &> /tmp/tmp.9dnpgxJCuE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits &> /tmp/tmp.8fUwLIOEKD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.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_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.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_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
Found non-empty wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
The reference image (wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits) and catalog (wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat) found
'wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.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 8106 out of 19207 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.937546
a=0.000000 b=1.000000 c=22.937546
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
2.1 pix Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
2.6 pix fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
2.6 pix fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
Limiting magnitude estimates:
15.3 mag. Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
15.3 mag. Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
14.1 mag. fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
14.1 mag. fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.4 (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.9sBGs61E8g (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1798, passed=19207
Got 19207 stars (including 17377 good ones) from the SExtractor catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 19207 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 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: 0.34"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.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.MhjSrKfKTL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits' -> 'wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
WCS-calibrated image found: wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
Checking if the catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
WCS catalog name: wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1805, passed=19223
Got 19223 stars (including 17389 good ones) from the SExtractor catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat
util/solve_plate_with_UCAC5 got 19223 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits -region wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.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.9dnpgxJCuE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
WCS_IMAGE_NAME=wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
WCS-calibrated image found: wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
Checking if the catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
WCS catalog name: wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=532, passed=7517
Got 7517 stars (including 6981 good ones) from the SExtractor catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat
util/solve_plate_with_UCAC5 got 7517 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.71"
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_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits -region wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.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.8fUwLIOEKD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
Checking if the catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
WCS catalog name: wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=516, passed=7353
Got 7353 stars (including 6833 good ones) from the SExtractor catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat
util/solve_plate_with_UCAC5 got 7353 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.75"
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_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits -region wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.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_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits'
Saving fully-calibrated image wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits'
Saving fully-calibrated image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits'
Saving fully-calibrated image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits'
Preparing the HTML report for the field Cam-11-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out16037.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 16037_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
Preparing report for the candidate 16037_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Cam-11-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 ####
04:19:08.31 +57:38:20.8
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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
SExtractor catalog cache: saved Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat to cache
SExtractor catalog cache: saved Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
Creating symlink local_wcs_cache/wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.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_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits exists and is non-empty
wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits exists and is non-empty
wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:14:05.422 +54:00:05.55
Second-epoch image center 04:14:06.659 +54:00:30.27
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:14:05.422 +54:00:05.55
Second-epoch image center 04:14:03.470 +54:00:43.50
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:14:06.659 +54:00:30.27
Second-epoch second image center 04:14:03.470 +54:00:43.50
Angular distance between the image centers 0.00863 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/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.MGVybu4cw2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits &> /tmp/tmp.AbGVwJwEJP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits &> /tmp/tmp.rnFlQiKkr3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits &> /tmp/tmp.QoNGojnmwy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.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_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.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_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
Found non-empty wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits and wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
The reference image (wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits) and catalog (wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat) found
'wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.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 8187 out of 141337 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779746
a=0.000000 b=1.000000 c=22.779746
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 74 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
2.0 pix Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
2.4 pix fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
2.4 pix fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
Limiting magnitude estimates:
15.5 mag. Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
15.5 mag. Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
14.3 mag. fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
14.2 mag. fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.7 (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.MGVybu4cw2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits' -> 'wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=15933, passed=141313
Got 141313 stars (including 125129 good ones) from the SExtractor catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 141313 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 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: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.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.AbGVwJwEJP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits' -> 'wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
WCS-calibrated image found: wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
Checking if the catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
WCS catalog name: wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=16037, passed=141692
Got 141692 stars (including 125423 good ones) from the SExtractor catalog wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat
util/solve_plate_with_UCAC5 got 141692 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits -region wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.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.rnFlQiKkr3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
WCS_IMAGE_NAME=wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
WCS-calibrated image found: wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
Checking if the catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
WCS catalog name: wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=3533, passed=54554
Got 54554 stars (including 50968 good ones) from the SExtractor catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat
util/solve_plate_with_UCAC5 got 54554 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits -region wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.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.QoNGojnmwy (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
WCS_IMAGE_NAME=wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
WCS-calibrated image found: wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
Checking if the catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat corresponding to the image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
WCS catalog name: wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3464, passed=53902
Got 53902 stars (including 50382 good ones) from the SExtractor catalog wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat
util/solve_plate_with_UCAC5 got 53902 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 966 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: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits -region wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.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_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/wcs_Cam-11-Q2b1x1_2026-01-17_20-32-37_20.00sec_-15.00C_LIGHT_0045.fits
Saving fully-calibrated image wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/wcs_Cam-11-Q2b1x1_2026-01-17_20-33-14_20.00sec_-15.00C_LIGHT_0046.fits
Saving fully-calibrated image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-41-38_20.00sec_-10.00C_LIGHT_0056.fits
Saving fully-calibrated image wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-11-Q2b1x1_214501_TTUQ2b1x1_14044_5EDiwG8A/wcs_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057.fits
Preparing the HTML report for the field Cam-11-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out162889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out162923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out163890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165554.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out166975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out167965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out168747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out169042.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out135811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44218.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: 2s
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Considering the candidate 162889_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162889_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:03:41.21 +51:40:59.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
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Considering the candidate 162891_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162891_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:29:52.56 +53:56:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162897_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162897_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:10:10.11 +53:23:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.524 275136159041754880 062.54254465188 +53.39931362505 13.1915 12.1715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162898_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162898_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:49:17.50 +53:38:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.672 273117627483328384 072.32354944685 +53.64210730509 13.6809 12.9624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162899_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162899_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:37:02.65 +57:35:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162904_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162904_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:44:51.56 +57:10:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162906_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162906_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:47:43.62 +55:07:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162907_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162907_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:46:20.12 +56:28:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162909_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162909_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:43:09.40 +49:47:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.755 259321986377607680 070.78934841075 +49.78714593481 12.8249 12.3912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162912_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162912_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:44:39.00 +55:06:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.432 274248097239381376 071.16239618408 +55.10518747607 13.3941 12.4386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 162913_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
Preparing report for the candidate 162913_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
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Considering the candidate 162914_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162914_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:46:04.34 +57:25:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162915_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162915_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:01:54.19 +56:35:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162916_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162916_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:19:34.93 +56:08:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162918_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162918_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:28:59.75 +53:48:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162921_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162921_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:53:08.14 +54:47:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162923_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 162923_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:15:20.97 +51:11:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 1.849 271668402446210816 063.83754052912 +51.19653090823 11.5544 11.2910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 163890_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 163890_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:26:46.60 +57:22:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 0.241 278433663129535360 066.69405394810 +57.36922166457 11.1223 10.5876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 163923_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 163923_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:18:05.06 +50:18:21.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165072_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 165072_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:20:05.85 +50:53:22.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165151_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 165151_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:46:52.44 +55:14:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 2.264 274244214588811776 071.71834173335 +55.24515028494 12.8603 12.2524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 165158_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 165158_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:22:02.50 +51:01:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.690 270774911807800704 065.50924417248 +51.02696245427 12.3066 11.5582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 165298_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 165298_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:08:27.63 +57:06:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 165554_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 165554_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:38:55.46 +49:55:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.262 258602970189538816 069.73162774196 +49.92524044806 12.3144 11.3446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 165602_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 165602_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:26:53.08 +51:58:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 0.820 271953412174451968 066.72148967965 +51.98308328438 11.8582 10.7290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 165910_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 165910_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:01:59.50 +49:54:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166407_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 166407_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:51:17.79 +54:55:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166512_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 166512_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:40:18.05 +51:05:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.402 260394869204487424 070.07620355511 +51.09134956701 12.2256 11.0888 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 166687_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 166687_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:15:09.49 +50:40:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166752_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 166752_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:19:04.00 +52:35:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166943_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 166943_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:56:08.42 +57:55:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166975_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 166975_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:40:15.64 +53:28:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.353 272978676705414528 070.06505122770 +53.47223558588 13.1341 12.4510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167336_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167336_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:40:17.86 +53:28:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.002 272978676705411712 070.07486676905 +53.47529278378 12.6700 11.5848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167390_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167390_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:22:11.51 +51:01:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.787 270774740008064512 065.54870151728 +51.02041680022 12.7970 11.8515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167409_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167409_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:50:55.20 +52:14:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 0.239 260936103804310784 072.72997185103 +52.23575867915 13.0060 12.2960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167429_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167429_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:47:01.81 +51:42:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167438_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167438_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:52:05.99 +52:45:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167535_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167535_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:13:36.05 +49:56:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167610_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167610_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:48:02.42 +55:34:58.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 167882_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167882_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:48:19.51 +52:03:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 167929_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167929_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:48:55.88 +50:41:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.641 251143200411524608 057.23269615956 +50.69137223876 12.9066 12.0598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167965_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 167965_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:28:33.49 +53:54:31.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
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Considering the candidate 168127_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 168127_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:15:20.29 +53:40:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.702 275204878518165760 063.83578662692 +53.68105468240 12.7747 11.6933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168286_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 168286_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:17:09.12 +53:23:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168339_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 168339_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:15:11.93 +53:43:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168376_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 168376_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:33:06.22 +55:28:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168472_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 168472_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:39:18.64 +51:37:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168517_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 168517_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:45:59.79 +50:25:02.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168747_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 168747_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:26:52.27 +52:00:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.124 271953725710817792 066.71643924510 +52.01516200098 13.8359 13.2774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168803_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 168803_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:35:47.13 +52:50:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168953_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 168953_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:51:28.33 +49:46:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169042_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 169042_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:41:42.18 +54:40:55.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169146_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 169146_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:02:15.75 +52:53:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.323 251839259992333568 060.56641535104 +52.89221240181 13.4320 12.8260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169152_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 169152_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:01:40.38 +53:50:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169203_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 169203_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:07:46.45 +51:25:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169234_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 169234_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:10:38.56 +57:50:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169451_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 169451_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:59:10.24 +58:01:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169841_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 169841_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:21:15.63 +56:43:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169899_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 169899_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:28:58.58 +54:35:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169998_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 169998_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:46:50.97 +55:13:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170160_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 170160_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:27:06.42 +51:11:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170753_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 170753_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:20:37.90 +51:07:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170906_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 170906_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:37:35.80 +52:52:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171599_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 171599_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:16:09.04 +56:26:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110796_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 110796_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:19:08.27 +57:38:20.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 27258_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
Preparing report for the candidate 27258_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
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Considering the candidate 75483_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 75483_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:06:12.25 +53:56:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156070_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 156070_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 04:31:04.89 +50:10:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140704_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 140704_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:34:55.94 +54:34:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 123505_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 123505_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
Rejecting candidate due to large distance (28.6") between the two second-epoch detections
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Considering the candidate 64609_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 64609_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks
**** FOUND 03:45:47.90 +52:38:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44218_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
Preparing report for the candidate 44218_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
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Considering the candidate 135811_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
Preparing report for the candidate 135811_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
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Considering the candidate 77359_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057
The candidate 77359_fd_Cam-11-Q2b1x1_2026-03-29_21-42-27_20.00sec_-10.00C_LIGHT_0057 did not pass the final checks