This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq
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
W Lyn,2461121.7790,11.96,0.05,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
W Lyn 20260322.2790 11.96CV 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:46.96 +40:07:51.7 ;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-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_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,2461121.7790,13.98,0.05,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 20260322.2790 13.98CV 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:01.16 +36:16:20.2 ;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-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_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,2461121.7790,14.49,0.05,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 20260322.2790 14.49CV 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:05:10.25 +36:00:41.9 ;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-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_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,2461121.7790,14.46,0.05,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 20260322.2790 14.46CV 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:32:50.68 +38:54:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_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,2461121.7790,14.59,0.05,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 20260322.2790 14.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:18:46.70 +33:28:57.9 ;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-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_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,2461121.7790,14.79,0.05,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 20260322.2790 14.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:54:36.90 +39:06:09.6 ;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-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20_00sec_-15_00C_LIGHT_0130_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20_00sec_-14_90C_LIGHT_0129_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: 2461032.98095582 23.12.2025 11:32:24.583 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
First image: 2461032.98095582 23.12.2025 11:32:24.583 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Last image: 2461121.77930307 22.03.2026 06:42:01.785 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 5 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): 10661
Objects passed selection criteria: 10657
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: 10388.2
Average stars matched: 10129.8 (97.5116 %)
Memory usage VmPeak: 116032 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 01:47:29 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: 2461032.98095582 23.12.2025 11:32:24.583 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
First image: 2461032.98095582 23.12.2025 11:32:24.583 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Last image: 2461121.77930307 22.03.2026 06:42:01.785 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 56
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
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: 20 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): 57276
Objects passed selection criteria: 57167
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: 55854.2
Average stars matched: 54007.8 (96.6941 %)
Memory usage VmPeak: 158980 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 01:48:40 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
SExtractor catalog cache: saved Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat to cache
SExtractor catalog cache: saved Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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: 2461121.77860875
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits exists and is non-empty
Saving wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits to local_wcs_cache/
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits' -> 'local_wcs_cache/wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits'
wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits exists and is non-empty
Saving wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits to local_wcs_cache/
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits' -> 'local_wcs_cache/wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits'
wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits exists and is non-empty
Saving wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits to local_wcs_cache/
'wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits' -> 'local_wcs_cache/wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits'
wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits exists and is non-empty
Saving wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits to local_wcs_cache/
'wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits' -> 'local_wcs_cache/wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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 08:43:38.316 +37:59:58.50
Second-epoch image center 08:43:38.716 +38:00:06.00
Angular distance between the image centers 0.00 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 08:43:38.316 +37:59:58.50
Second-epoch image center 08:43:36.081 +37:59:29.88
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 08:43:38.716 +38:00:06.00
Second-epoch second image center 08:43:36.081 +37:59:29.88
Angular distance between the image centers 0.01325 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits &> /tmp/tmp.sp8HWuG3LE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits &> /tmp/tmp.GbWLZL0F8o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits &> /tmp/tmp.OOhTVPPmoI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits &> /tmp/tmp.e1JgCRjcPw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
Found non-empty wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
The reference image (wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits) and catalog (wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat) found
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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 5313 out of 10418 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.940274
a=0.000000 b=1.000000 c=22.940274
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
2.1 pix Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
2.1 pix fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
2.3 pix fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
Limiting magnitude estimates:
15.5 mag. Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
15.5 mag. Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
15.4 mag. fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
15.4 mag. fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
All-image limiting magnitude estimate: 15.4 (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.sp8HWuG3LE (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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits' -> 'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS-calibrated image found: wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Checking if the catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS catalog name: wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=693, passed=10418
Got 10418 stars (including 9715 good ones) from the SExtractor catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
util/solve_plate_with_UCAC5 got 10418 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits -region wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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.GbWLZL0F8o (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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits' -> 'wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS-calibrated image found: wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Checking if the catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS catalog name: wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=705, passed=10485
Got 10485 stars (including 9770 good ones) from the SExtractor catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat
util/solve_plate_with_UCAC5 got 10485 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 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: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits -region wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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.OOhTVPPmoI (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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
Checking if the catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
WCS catalog name: wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=622, passed=10267
Got 10267 stars (including 9632 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat
util/solve_plate_with_UCAC5 got 10267 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 977 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 977 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: 0.30"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits -region wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.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.e1JgCRjcPw (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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
Checking if the catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
WCS catalog name: wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=560, passed=10577
Got 10577 stars (including 10005 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat
util/solve_plate_with_UCAC5 got 10577 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 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits -region wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits'
Saving fully-calibrated image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits'
Saving fully-calibrated image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits'
Saving fully-calibrated image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits'
Preparing the HTML report for the field Lyn-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03008.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 20587_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 20587_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:05:19.97 +38:25:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 1.267 719023567400007808 136.33325965572 +38.43193309666 12.4615 11.8207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20588_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 20588_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:45:20.74 +38:50:28.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20590_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 20590_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:45:30.68 +38:11:10.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20592_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 20592_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:09:45.42 +39:06:34.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20593_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 20593_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:51:47.75 +38:13:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.049 719739113248220928 132.94876763809 +38.22311117408 12.3395 11.7770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20594_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 20594_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:54:22.22 +36:48:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.415 717189448862453760 133.59253009587 +36.80480143600 12.4260 11.7637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20595_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 20595_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:39:39.90 +38:34:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.142 910651612145244416 129.91630020902 +38.58291881855 12.4495 11.9768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04725_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 04725_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:28:07.99 +38:20:22.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03008_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
Preparing report for the candidate 03008_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00780_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 00780_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:08:47.75 +42:09:19.9 in the exclusion list exclusion_list.txt ****
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-06-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 ####
08:16:46.96 +40:07:51.7
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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
SExtractor catalog cache: saved Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat to cache
SExtractor catalog cache: saved Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Creating symlink local_wcs_cache/wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits exists and is non-empty
wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits exists and is non-empty
wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits exists and is non-empty
wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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 08:43:38.316 +37:59:58.50
Second-epoch image center 08:43:38.716 +38:00:06.00
Angular distance between the image centers 0.00 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 08:43:38.316 +37:59:58.50
Second-epoch image center 08:43:36.081 +37:59:29.88
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 08:43:38.716 +38:00:06.00
Second-epoch second image center 08:43:36.081 +37:59:29.88
Angular distance between the image centers 0.01325 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits &> /tmp/tmp.KBjzy6MCqm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits &> /tmp/tmp.ObbN87Wsdp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits &> /tmp/tmp.jlVQrbOrdp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits &> /tmp/tmp.8pvLn2p1Is
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
Found non-empty wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
The reference image (wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits) and catalog (wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat) found
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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 5344 out of 57791 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.838131
a=0.000000 b=1.000000 c=22.838131
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
2.0 pix Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
2.0 pix fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
2.3 pix fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
Limiting magnitude estimates:
15.6 mag. Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
15.6 mag. Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
15.6 mag. fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
15.5 mag. fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.8 (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.KBjzy6MCqm (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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits' -> 'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS-calibrated image found: wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Checking if the catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS catalog name: wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3024, passed=57768
Got 57768 stars (including 54668 good ones) from the SExtractor catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
util/solve_plate_with_UCAC5 got 57768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits -region wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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.ObbN87Wsdp (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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits' -> 'wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS-calibrated image found: wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Checking if the catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS catalog name: wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=3079, passed=57501
Got 57501 stars (including 54340 good ones) from the SExtractor catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat
util/solve_plate_with_UCAC5 got 57501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 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: 0.32"
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 977 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: 0.29"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits -region wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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.jlVQrbOrdp (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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
Checking if the catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
WCS catalog name: wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=2746, passed=56200
Got 56200 stars (including 53374 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat
util/solve_plate_with_UCAC5 got 56200 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 977 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 977 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 - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits -region wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.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.8pvLn2p1Is (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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
Checking if the catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
WCS catalog name: wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=2653, passed=53127
Got 53127 stars (including 50388 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat
util/solve_plate_with_UCAC5 got 53127 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 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Lyn-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits -region wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Saving fully-calibrated image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Saving fully-calibrated image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-41-01_20.00sec_-14.90C_LIGHT_0129.fits
Saving fully-calibrated image wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.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-06-Q1b1x1_014241_TTUQ1b1x1_16491_npf5wCZq/wcs_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130.fits
Preparing the HTML report for the field Lyn-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out71715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71921.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72243.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out72383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out71909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72172.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 71715_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71715_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:19:33.03 +42:55:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.812 915892503038723712 124.88825141895 +42.91857059969 14.9978 14.5272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71718_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71718_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:51:49.20 +36:42:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.203 717909319741423232 132.95460630416 +36.71291503069 15.0421 14.5643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71723_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71723_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:13:49.80 +39:56:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.75, MAG_FAINT_SEARCH_LIMIT=15.73)GAIADR2_OUTPUT=# 1.102 909481594334650112 123.45713732083 +39.93570509092 14.5320 13.8501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71725_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71725_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:06:42.14 +41:46:58.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71726_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71726_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:07:38.29 +34:55:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 0.955 714995407769350400 136.90930206010 +34.93295620002 14.7719 14.2079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71727_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71727_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:25:55.16 +38:59:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 1.251 914250554221311360 126.48024844827 +38.98818492306 14.5679 13.8168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71875_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71875_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:07:07.62 +38:21:49.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71909_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
Preparing report for the candidate 71909_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71921_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71921_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:38:38.40 +34:30:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.355 711251364518611072 129.66048001230 +34.50557658090 14.1591 13.6759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71930_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71930_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:31:33.13 +33:35:07.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71947_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71947_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:08:27.00 +39:57:50.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71954_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71954_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:39:22.33 +41:56:12.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71995_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 71995_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:27:25.47 +41:42:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.508 915153493785664768 126.85560279369 +41.70184739313 14.5648 14.0597 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72014_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
Preparing report for the candidate 72014_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72053_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
Preparing report for the candidate 72053_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72065_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72065_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:06:23.79 +34:24:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 1.958 714204618390481536 136.59866797148 +34.41350321197 14.6934 14.0970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.958#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72078_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72078_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:32:04.03 +35:35:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 1.594 903673870837456640 128.01715687171 +35.58660603144 14.5416 14.0649 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 72099_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
Preparing report for the candidate 72099_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72103_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72103_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:07:16.90 +34:47:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 1.368 905874440281145472 121.82002011564 +34.78686222331 14.6810 14.2204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72105_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72105_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:07:57.64 +34:48:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.66, MAG_FAINT_SEARCH_LIMIT=15.64)GAIADR2_OUTPUT=# 0.799 905863548244073344 121.99039424173 +34.80968555031 14.7163 14.2400 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72117_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72117_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:36:46.42 +42:36:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 1.766 916564407722239616 129.19302140929 +42.60377171521 14.8003 14.2636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72134_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72134_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:52:17.08 +42:01:29.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72172_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
Preparing report for the candidate 72172_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72187_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72187_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:06:02.92 +34:15:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.603 905447245654126976 121.51230046977 +34.26284646969 14.6013 13.8581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72198_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72198_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:22:00.59 +40:26:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 0.171 812764943783561472 140.50239962044 +40.44532139703 15.0454 14.5565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72224_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72224_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:50:54.47 +39:07:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 1.519 719861708794568448 132.72657174287 +39.12936997278 15.1783 14.6543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72228_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72228_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:08:32.54 +33:53:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.462 902396581923992192 122.13517493114 +33.89519325406 14.8006 14.2640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72231_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72231_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:00:15.84 +33:04:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 0.226 713264982625501312 135.06599466844 +33.07795163344 14.8515 14.3595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72243_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72243_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:55:31.09 +42:02:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 1.314 912785558056894336 133.88002718691 +42.04555410663 14.8667 14.3389 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72245_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72245_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:59:50.33 +39:44:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=15.00, MAG_FAINT_SEARCH_LIMIT=15.98)GAIADR2_OUTPUT=# 0.439 720126656736950784 134.95981612151 +39.74974399381 15.2775 14.7360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72246_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72246_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:39:54.42 +42:25:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.270 913523605236531328 129.97696487416 +42.41943496491 15.1503 14.6580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72276_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72276_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:11:42.33 +35:53:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.936 906038714190164480 122.92631840551 +35.88679957733 14.8060 14.1618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72282_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72282_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:15:46.12 +42:25:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=15.00, MAG_FAINT_SEARCH_LIMIT=15.98)GAIADR2_OUTPUT=# 0.524 816210744505137280 138.94197006666 +42.41892883393 14.9422 14.3988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72299_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72299_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:13:20.83 +42:49:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 0.480 927864741556392960 123.33691937942 +42.83198855822 14.8497 14.2488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72307_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72307_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:23:58.77 +39:20:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 2.042 812379393159970816 140.99537762548 +39.33819816218 15.0346 14.4398 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 72310_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72310_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:23:50.26 +41:25:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.728 915511453540158464 125.95950486674 +41.42161436453 14.8770 14.1554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72318_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72318_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:09:53.65 +35:03:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 2.267 905847364807261568 122.47282646423 +35.05776816600 15.2320 14.5709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72349_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72349_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:20:44.67 +38:32:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.158 908176989427971840 125.18582583611 +38.53677633563 14.9113 14.3990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72355_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72355_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:39:47.97 +40:36:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.671 911683263289424256 129.94941066260 +40.60703131254 15.2075 14.7604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72383_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 72383_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:08:15.25 +39:46:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.001 909151259809849472 122.06325152351 +39.77713960429 14.8338 14.3833 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 69696_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 69696_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:40:41.28 +42:36:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16581_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 16581_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 08:16:46.98 +40:07:51.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03975_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 03975_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks
**** FOUND 09:08:47.74 +42:09:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27063_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130
The candidate 27063_fd_Lyn-06-Q1b1x1_2026-03-22_01-42-01_20.00sec_-15.00C_LIGHT_0130 did not pass the final checks