This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3
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
XX Gem,2461121.7587,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
XX Gem 20260322.2587 10.58CV 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/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:26:13.59 +33:22:21.7 ;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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7587,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2587 14.13CV 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/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:27:28.66 +36:35:36.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7587,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2587 14.38CV 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/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:13.92 +34:25:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7587,14.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260322.2587 14.72CV 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/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:57:52.03 +33:20:02.9 ;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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_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
RW Lyn,2461121.7587,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
RW Lyn 20260322.2587 12.27CV 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/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:50:39.24 +38:27:13.9 ;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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20_00sec_-14_90C_LIGHT_0102_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20_00sec_-14_90C_LIGHT_0101_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: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
First image: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Last image: 2461121.75907297 22.03.2026 06:12:53.905 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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: 7 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): 16938
Objects passed selection criteria: 16932
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 16428.8
Average stars matched: 16118.5 (98.1115 %)
Memory usage VmPeak: 121328 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 22 01:21:04 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: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
First image: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Last image: 2461121.75907297 22.03.2026 06:12:53.905 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 73
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 45 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): 97380
Objects passed selection criteria: 97153
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 93975.8
Average stars matched: 91253.2 (97.103 %)
Memory usage VmPeak: 2187792 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 22 01:22:50 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
SExtractor catalog cache: saved Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.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/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.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: 2461121.75828463
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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits exists and is non-empty
Saving wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits to local_wcs_cache/
'wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits exists and is non-empty
Saving wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits to local_wcs_cache/
'wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits'
wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.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 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:11.063 +37:59:55.78
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 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:13.598 +37:59:26.59
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 07:38:11.063 +37:59:55.78
Second-epoch second image center 07:38:13.598 +37:59:26.59
Angular distance between the image centers 0.01162 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/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits &> /tmp/tmp.6VV42ZT2v6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits &> /tmp/tmp.tWbv8E8Vyz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits &> /tmp/tmp.TlgbBbQEXf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits &> /tmp/tmp.jroURIkZWz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Found non-empty wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
The reference image (wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits) and catalog (wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat) found
'wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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 7689 out of 17251 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.958948
a=0.000000 b=1.000000 c=22.958948
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
2.2 pix Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
2.2 pix fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
2.2 pix fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
Limiting magnitude estimates:
15.5 mag. Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
15.5 mag. Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
15.3 mag. fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
15.3 mag. fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.4 (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.6VV42ZT2v6 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> 'wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS-calibrated image found: wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Checking if the catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS catalog name: wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1370, passed=17251
Got 17251 stars (including 15857 good ones) from the SExtractor catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
util/solve_plate_with_UCAC5 got 17251 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits -region wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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.tWbv8E8Vyz (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> 'wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS-calibrated image found: wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Checking if the catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS catalog name: wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1310, passed=17199
Got 17199 stars (including 15864 good ones) from the SExtractor catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
util/solve_plate_with_UCAC5 got 17199 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 956 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits -region wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.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.TlgbBbQEXf (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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
Checking if the catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1057, passed=15871
Got 15871 stars (including 14794 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat
util/solve_plate_with_UCAC5 got 15871 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits -region wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.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.jroURIkZWz (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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
Checking if the catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
WCS catalog name: wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1096, passed=15802
Got 15802 stars (including 14686 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat
util/solve_plate_with_UCAC5 got 15802 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits -region wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
Saving fully-calibrated image wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits'
Preparing the HTML report for the field Lyn-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out14539.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 20985_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 20985_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:50:39.27 +38:27:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.070 920040926051061248 117.66325682540 +38.45398841232 12.9177 12.4854 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20991_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 20991_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:44:34.49 +36:39:11.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20992_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 20992_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:48:01.95 +35:33:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20994_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 20994_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:40:48.16 +38:01:06.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20996_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 20996_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:46:58.26 +41:40:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 2.162 923939656843716992 116.74247141751 +41.67561902418 12.3767 11.7814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14539_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
Preparing report for the candidate 14539_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Lyn-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:26:13.59 +33:22:21.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
SExtractor catalog cache: saved Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Creating symlink local_wcs_cache/wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits exists and is non-empty
wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits exists and is non-empty
wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits exists and is non-empty
wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.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 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:11.063 +37:59:55.78
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 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:13.598 +37:59:26.59
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 07:38:11.063 +37:59:55.78
Second-epoch second image center 07:38:13.598 +37:59:26.59
Angular distance between the image centers 0.01162 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/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits &> /tmp/tmp.b47x8uvTSv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits &> /tmp/tmp.dCZbacDzrC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits &> /tmp/tmp.VcctFmWTi4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits &> /tmp/tmp.alZEUf7jyS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Found non-empty wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
The reference image (wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits) and catalog (wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat) found
'wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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 7746 out of 100375 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.850461
a=0.000000 b=1.000000 c=22.850461
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 54 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
2.0 pix Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
2.2 pix fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
2.2 pix fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
Limiting magnitude estimates:
15.6 mag. Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
15.6 mag. Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
15.4 mag. fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
15.4 mag. fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (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.b47x8uvTSv (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> 'wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS-calibrated image found: wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Checking if the catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS catalog name: wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=7665, passed=100350
Got 100350 stars (including 92512 good ones) from the SExtractor catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
util/solve_plate_with_UCAC5 got 100350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 953 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits -region wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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.dCZbacDzrC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> 'wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS-calibrated image found: wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Checking if the catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS catalog name: wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=7582, passed=100415
Got 100415 stars (including 92657 good ones) from the SExtractor catalog wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
util/solve_plate_with_UCAC5 got 100415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 951 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: 0.36"
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 951 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: 0.34"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits -region wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.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.VcctFmWTi4 (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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
Checking if the catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=6197, passed=88807
Got 88807 stars (including 82488 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat
util/solve_plate_with_UCAC5 got 88807 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits -region wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.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.alZEUf7jyS (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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
Checking if the catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
WCS catalog name: wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6169, passed=88623
Got 88623 stars (including 82296 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat
util/solve_plate_with_UCAC5 got 88623 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits -region wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.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_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/wcs_Lyn-05-Q1b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Saving fully-calibrated image wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/wcs_Lyn-05-Q1b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-11-45_20.00sec_-14.90C_LIGHT_0101.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.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_2026-03-22_CI_Lyn-05-Q1b1x1_011341_TTUQ1b1x1_26618_JsgsmmS3/wcs_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102.fits
Preparing the HTML report for the field Lyn-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out118035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118524.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118651.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out118343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118571.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43178.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118035_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118035_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:39:43.35 +34:29:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 2.125 894315480697255936 114.93045354250 +34.49210094228 14.7908 14.3334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118043_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118043_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:54:35.08 +36:04:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 4.414 906760715372994688 118.64466154465 +36.07031998752 14.9198 14.3216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118052_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118052_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 08:03:30.66 +42:11:33.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118054_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118054_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:22:56.44 +33:29:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 2.042 893339939005585408 110.73511718437 +33.48603800946 14.7304 14.2255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118055_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118055_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:21:39.47 +40:38:46.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 0.362 948268791150177920 110.41457623323 +40.64621253707 14.1858 13.5497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118067_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118067_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:04:06.33 +39:50:29.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118075_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118075_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:28:16.13 +33:29:25.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118076_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118076_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:30:05.38 +35:19:21.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118207_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118207_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:23:15.86 +35:10:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.653 896880194648481024 110.81579219150 +35.17908721532 13.3992 12.8456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118230_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118230_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:06:07.60 +34:26:34.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118237_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118237_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:08:26.88 +33:15:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.332 891165964000305024 107.11238212155 +33.25670236122 13.5543 12.9012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.332#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118309_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118309_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 08:01:10.92 +37:23:16.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118321_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118321_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:47:41.15 +33:25:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 2.159 882055479371076096 116.92209689459 +33.41760811613 14.0292 12.9775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118343_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
Preparing report for the candidate 118343_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118353_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118353_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:56:38.09 +36:53:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.800 918911590170434688 119.15778575843 +36.89814272919 14.3978 13.9474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118390_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118390_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:08:07.39 +38:16:35.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118394_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118394_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:11:56.71 +35:10:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 4.310 897443178962091776 107.98546771893 +35.17442674097 14.2069 13.5621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118401_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
Preparing report for the candidate 118401_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118415_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118415_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:13:17.50 +33:19:27.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118421_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118421_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:18:47.66 +33:52:56.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118511_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118511_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:02:13.48 +37:41:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 0.720 946910825570526080 105.55632692486 +37.69696012574 14.5786 14.0979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118524_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118524_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 06:58:57.96 +39:18:47.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118534_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118534_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:00:08.08 +41:26:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 0.618 951116698065343872 105.03369595574 +41.44825365221 14.7653 14.1727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.618#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118546_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118546_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:03:37.82 +33:57:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 2.371 891455410435948544 105.90744040557 +33.95195349419 14.7676 14.1235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118562_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118562_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:37:27.33 +37:14:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.701 896021991463639168 114.36409847541 +37.24552108280 14.8704 14.3613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118566_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118566_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118571_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
Preparing report for the candidate 118571_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118579_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118579_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:03:23.15 +37:21:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.477 946137731457427200 105.84612312155 +37.35128406504 14.7599 14.0838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118591_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118591_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 08:16:23.31 +42:02:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.594 915738674489893760 124.09665108012 +42.04157410799 15.3257 14.8314 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118598_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118598_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:15:12.40 +32:58:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 0.754 890264295745242752 108.80165280719 +32.97440203972 14.8487 14.4596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118600_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118600_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:35:48.09 +43:04:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 0.876 925232613799190144 113.95032470840 +43.06826834100 14.6504 13.8134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118617_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118617_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:01:33.02 +39:01:04.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118618_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118618_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 08:03:38.47 +32:49:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.965 881204594810125824 120.91008034115 +32.82325643053 14.9116 14.3512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.965#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118619_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118619_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 08:00:44.58 +33:55:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 2.122 905532492164818048 120.18504490332 +33.92576524584 15.0626 14.6050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118622_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118622_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:02:01.71 +42:20:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 2.942 951281590449940480 105.50649010992 +42.34266440257 15.1844 14.6966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118637_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118637_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:10:43.67 +40:22:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 0.615 947693471691481728 107.68218220606 +40.36878850698 14.7141 14.2528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118642_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118642_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:24:55.44 +33:17:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 2.117 893289979946096896 111.23158770267 +33.29473247177 14.8456 14.5077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118644_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118644_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:24:53.83 +42:33:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 0.457 949041438586920064 111.22437916592 +42.55722061757 14.8297 14.2690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118651_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118651_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:10:04.99 +33:16:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.630 890438877576371968 107.52032261518 +33.26958766412 14.7347 14.2078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118662_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118662_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:06:26.03 +36:42:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.827 945860001691588864 106.60865662209 +36.70488809943 14.7811 14.3093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118671_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118671_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:00:34.62 +34:07:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.409 939183870167167360 105.14435747775 +34.12726527041 14.8734 14.3366 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118690_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118690_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 08:08:34.15 +42:31:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.512 922005615890799360 122.14257052231 +42.51897739718 14.9091 14.4002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118698_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118698_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:29:47.14 +37:26:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 3.244 898898348241312896 112.44586328931 +37.44106459484 15.2058 14.7064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118716_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118716_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:14:51.84 +38:39:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 0.670 946543653110133632 108.71576362089 +38.65417105853 14.8960 14.2756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118740_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118740_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:14:15.13 +34:31:08.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118763_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118763_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:12:39.34 +42:45:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 1.525 949619231946806272 108.16335011916 +42.76369785106 14.8287 14.1969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118768_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118768_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 08:03:52.49 +39:21:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.886 921019972435852160 120.96902628437 +39.36212152452 14.9645 14.4895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118822_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118822_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:20:44.33 +37:13:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 0.174 898132022996133120 110.18469628321 +37.22071416979 15.0179 14.4535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.174#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118840_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118840_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:17:16.05 +34:27:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 3.051 896566279783519872 109.31733216535 +34.45592579000 15.2030 14.5624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118865_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118865_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:17:57.91 +35:07:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.281 896738185850155776 109.49085714151 +35.13034864982 15.2249 14.7802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118880_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118880_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:07:00.67 +38:23:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 2.502 946308636795932416 106.75204418509 +38.38873733286 14.9180 14.3661 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118887_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 118887_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks
**** FOUND 07:20:50.90 +33:05:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.378 893245003048443904 110.21195735225 +33.08967350065 14.8441 14.2778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43178_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
Preparing report for the candidate 43178_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64977_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102
The candidate 64977_fd_Lyn-05-Q1b1x1_2026-03-22_01-12-53_20.00sec_-14.90C_LIGHT_0102 did not pass the final checks