This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr
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!
TCP 2026 03 22.2729* 09 43 31.88 +17 07 40.4 13.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7729,13.09,0.05,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 20260322.2729 13.09CV 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:43:31.88 +17:07:40.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_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,2461121.7729,13.30,0.05,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 20260322.2729 13.30CV 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:47:46.80 +19:32:24.3 ;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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2729* 09 22 37.89 +20 00 43.6 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7729,13.77,0.05,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 20260322.2729 13.77CV 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:22:37.89 +20:00:43.6 ;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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2729* 09 46 50.09 +26 39 07.5 14.1 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7729,14.07,0.05,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 20260322.2729 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:46:50.09 +26:39:07.5 ;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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2729* 09 23 23.79 +25 31 12.5 14.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7729,14.04,0.05,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 20260322.2729 14.04CV 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:23:23.79 +25:31:12.5 ;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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_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,2461121.7729,14.05,0.05,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 20260322.2729 14.05CV 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:02:22.10 +22:29:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_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,2461121.7729,14.19,0.05,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 20260322.2729 14.19CV 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:38.07 +22:10:44.2 ;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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_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,2461121.7729,14.19,0.05,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 20260322.2729 14.19CV 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:42:31.23 +19:57:30.5 ;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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_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,2461121.7729,14.46,0.05,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 20260322.2729 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:59:24.58 +22:54:24.5 ;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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2729* 09 43 33.17 +23 05 44.9 14.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7729,14.79,0.05,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 20260322.2729 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:43:33.17 +23:05:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_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,2461121.7729,14.85,0.05,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 20260322.2729 14.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:48.92 +21:12:07.2 ;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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_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,2461121.7729,14.81,0.05,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 20260322.2729 14.81CV 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:00:58.69 +18:01:03.2 ;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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20_00sec_-15_00C_LIGHT_0121_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: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
First image: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Last image: 2461121.77326444 22.03.2026 06:33:20.048 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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): 9302
Objects passed selection criteria: 9297
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: 8987.25
Average stars matched: 8599 (95.68 %)
Memory usage VmPeak: 114892 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 01:37:07 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: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
First image: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Last image: 2461121.77326444 22.03.2026 06:33:20.048 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 107
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
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: 22 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): 50069
Objects passed selection criteria: 49945
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: 48935
Average stars matched: 46706.8 (95.4465 %)
Memory usage VmPeak: 149408 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 01:38:12 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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: 2461121.77261594
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits exists and is non-empty
Saving wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits exists and is non-empty
Saving wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits'
wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:13:50.826 +21:59:57.24
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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:13:48.006 +21:59:50.72
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 09:13:50.826 +21:59:57.24
Second-epoch second image center 09:13:48.006 +21:59:50.72
Angular distance between the image centers 0.01104 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits &> /tmp/tmp.JoFS1RYAF4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits &> /tmp/tmp.2eDRi46K78
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits &> /tmp/tmp.nqNsGuQDrl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits &> /tmp/tmp.mlNIbGUhCL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
Found non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
The reference image (wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits) and catalog (wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat) found
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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 4769 out of 8632 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.930105
a=0.000000 b=1.000000 c=22.930105
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
2.1 pix Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
2.1 pix fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
2.2 pix fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
Limiting magnitude estimates:
15.3 mag. Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
15.3 mag. Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
15.4 mag. fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
15.4 mag. fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 12.3 (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.JoFS1RYAF4 (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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> 'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=673, passed=8632
Got 8632 stars (including 7938 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
util/solve_plate_with_UCAC5 got 8632 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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits -region wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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.2eDRi46K78 (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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> 'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=654, passed=8532
Got 8532 stars (including 7867 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
util/solve_plate_with_UCAC5 got 8532 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 956 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 - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits -region wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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.nqNsGuQDrl (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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=609, passed=9494
Got 9494 stars (including 8870 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat
util/solve_plate_with_UCAC5 got 9494 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 956 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: 0.26"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.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.mlNIbGUhCL (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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=602, passed=9574
Got 9574 stars (including 8959 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat
util/solve_plate_with_UCAC5 got 9574 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 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: 0.25"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
Saving fully-calibrated image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits'
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20471.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20470_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 20470_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:46:46.90 +23:21:58.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20471_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 20471_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:19:28.91 +25:10:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.217 687642272888501504 139.87040190261 +25.16894846649 12.3732 11.9184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20472_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 20472_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:16:41.19 +21:02:12.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20473_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 20473_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:12:25.42 +22:01:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20474_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 20474_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:24:31.88 +22:49:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20476_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 20476_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:26:33.78 +24:12:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20477_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 20477_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:30:45.44 +20:14:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01624_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 01624_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:09:52.55 +25:14:52.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cnc-03-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 ####
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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits exists and is non-empty
wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:13:50.826 +21:59:57.24
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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:13:48.006 +21:59:50.72
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 09:13:50.826 +21:59:57.24
Second-epoch second image center 09:13:48.006 +21:59:50.72
Angular distance between the image centers 0.01104 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/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits &> /tmp/tmp.4DLTmFy6w8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits &> /tmp/tmp.FLH4ozSeyk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits &> /tmp/tmp.KGWDcuHsM8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits &> /tmp/tmp.8uECe2xoEm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
Found non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
The reference image (wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits) and catalog (wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat) found
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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 4825 out of 48025 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.818214
a=0.000000 b=1.000000 c=22.818214
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 85 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
2.0 pix Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
2.1 pix fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
2.1 pix fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
Limiting magnitude estimates:
15.5 mag. Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
15.4 mag. Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
15.6 mag. fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
15.5 mag. fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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.4DLTmFy6w8 (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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> 'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
SExtractor catalog parsing summary: zero_flux=11, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2316, passed=47999
Got 47999 stars (including 45610 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
util/solve_plate_with_UCAC5 got 47999 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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits -region wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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.FLH4ozSeyk (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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> 'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=2292, passed=48027
Got 48027 stars (including 45647 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
util/solve_plate_with_UCAC5 got 48027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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 957 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: 0.33"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits -region wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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.KGWDcuHsM8 (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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2356, passed=50780
Got 50780 stars (including 48344 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat
util/solve_plate_with_UCAC5 got 50780 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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 954 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: 0.28"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.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.8uECe2xoEm (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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2361, passed=50090
Got 50090 stars (including 47650 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat
util/solve_plate_with_UCAC5 got 50090 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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 954 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 - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Saving fully-calibrated image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-32-24_20.00sec_-15.00C_LIGHT_0121.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.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_Cnc-03-Q1b1x1_013411_TTUQ1b1x1_22212_7kgAkAzr/wcs_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122.fits
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53575.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53746.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out53857.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out53497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53656.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54013.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 8s
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Considering the candidate 53426_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53426_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:05:35.81 +21:29:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 0.116 685217368712277504 136.39917372782 +21.48733187736 14.8525 12.9407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53427_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53427_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:57:27.65 +21:42:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 2.995 685828319221304320 134.36435727718 +21.70436964664 14.7629 14.2024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53430_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53430_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:19:53.60 +24:55:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=15.00, MAG_FAINT_SEARCH_LIMIT=15.98)GAIADR2_OUTPUT=# 1.767 687622516038947072 139.97296649452 +24.92730588285 15.1414 14.6297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53431_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53431_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:54:51.67 +26:53:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.595 692544376762465280 133.71507347535 +26.88985208913 15.0574 14.2970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53432_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53432_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:12:09.12 +24:25:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 0.532 687718482788877952 138.03814872917 +24.42180161539 14.6845 13.7297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53433_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53433_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:00:15.39 +22:54:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.566 686348937976746752 135.06416596899 +22.91568036395 15.0359 14.6299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53435_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53435_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:06:55.38 +23:27:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 0.614 687179206695101184 136.73073804528 +23.45078134863 14.5323 13.8764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53437_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53437_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:44:40.25 +25:00:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.980 690634215827559552 131.16762415221 +25.00198855815 14.4716 14.0422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53442_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53442_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:22:48.72 +17:19:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 0.749 632208126430886144 140.70280740699 +17.32237492756 13.8086 13.3122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53497_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53497_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53521_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53521_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53523_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53523_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:42:15.78 +24:29:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.835 644751561238913280 145.56551707203 +24.48826662228 13.3509 12.7256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53546_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53546_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:43:05.02 +19:27:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 0.873 661043918382057344 130.77072810799 +19.45819253245 13.4435 12.6433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53575_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53575_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:30:55.63 +24:06:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.182 645283449989164160 142.73181941765 +24.10667269500 13.9755 13.3651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53580_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53580_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53597_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53597_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53625_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53625_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53629_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53629_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53656_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53656_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53664_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53664_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:40:23.46 +26:13:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53677_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53677_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:11:41.25 +26:18:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.134 688924990642068480 137.92189630380 +26.30718545586 14.6620 14.0682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53685_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53685_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:54:31.87 +22:50:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53688_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53688_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53703_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53703_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:43:08.13 +21:10:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53746_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53746_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:38:24.28 +17:02:41.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)
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Considering the candidate 53747_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53747_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:43:23.26 +20:36:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53749_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53749_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53751_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53751_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:45:03.09 +22:34:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)GAIADR2_OUTPUT=# 0.458 641233811224835200 146.26278538840 +22.57870773747 14.6463 13.9378 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53763_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53763_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:43:34.60 +26:23:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 5.819 646760884378972416 145.89285889489 +26.39346966287 15.2612 14.6072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53789_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53789_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:50:29.65 +17:02:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53816_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53816_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:46:44.10 +19:00:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53819_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53819_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:19:10.39 +26:57:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 0.459 694842287344893696 139.79322276045 +26.95930484377 15.4060 15.0298 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53822_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53822_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:40:10.92 +17:00:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.997 620606384676811136 145.04603136981 +17.01002807198 14.9708 14.4161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53832_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53832_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:51:07.42 +21:13:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.184 661744616526136448 132.78062289288 +21.22740424709 14.6567 13.9974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53838_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53838_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:17:01.18 +19:07:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.470 635690417195197696 139.25448443844 +19.13256227645 14.8569 14.3233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53853_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53853_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:59:54.14 +18:48:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 2.306 612383828703560832 134.97541582838 +18.80759295559 15.1357 14.6302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53857_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53857_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:02:44.04 +25:25:15.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)
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Considering the candidate 53858_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53858_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53861_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53861_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:37:44.37 +16:49:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.850 620693697067723136 144.43540375837 +16.83058890203 14.9153 14.4298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53868_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53868_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:53:05.10 +24:50:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 2.059 689963582453701632 133.27068721703 +24.84349258486 14.8388 14.3321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53874_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 53874_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 53880_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53880_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:55:34.46 +22:46:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 2.162 686158413227666560 133.89317171792 +22.77752116155 14.9407 14.3961 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53885_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53885_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:46:38.51 +20:37:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 2.022 661800549884160384 131.65994742615 +20.62128884170 14.9738 14.4668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53886_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53886_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:42:00.60 +25:48:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.152 702741591196083456 130.50224742213 +25.81169152032 14.7146 14.2244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53891_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53891_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:44:59.15 +17:02:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 0.824 620935452186833664 146.24626423954 +17.04656056904 14.9567 14.4550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53894_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53894_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:04:12.44 +21:44:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.207 685427169275847936 136.05155217619 +21.74745633075 14.8716 14.3506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.207#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53895_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53895_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:41:52.96 +16:59:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.363 658419968241995264 130.47041908234 +16.98942664937 14.7434 14.2861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53899_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53899_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:42:56.17 +22:16:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.75, MAG_FAINT_SEARCH_LIMIT=15.73)GAIADR2_OUTPUT=# 2.869 665274220650812672 130.73387383165 +22.26985713438 14.7475 14.2547 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53904_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53904_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:46:05.85 +21:46:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.822 665011884048135808 131.52417768185 +21.78335856751 14.7830 14.2269 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53917_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53917_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:31:29.70 +17:49:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.543 633047569198903680 142.87339372780 +17.83118220323 15.0913 14.5220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.543#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53925_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53925_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:45:35.07 +21:08:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.455 661884013985032192 131.39608477629 +21.14985156654 14.8768 14.3251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53926_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53926_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:34:54.92 +21:52:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 0.489 640994152049784960 143.72896898884 +21.86711544756 14.8773 14.4038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53931_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53931_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:02:32.06 +17:53:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.419 612087952700772992 135.63317370747 +17.88847591533 14.8440 14.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53933_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53933_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:50:16.70 +22:33:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.202 689092769244173824 132.56924164630 +22.55644600202 14.7014 14.2771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53935_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53935_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:46:26.48 +21:35:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 1.173 664994532380267136 131.60998808150 +21.58936083830 14.7905 14.1106 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53940_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53940_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:01:16.91 +17:51:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 2.064 611996766250525312 135.32027934420 +17.86231354575 14.7238 13.8145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53946_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53946_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:50:01.87 +20:54:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 2.538 661708878102149504 132.50706249716 +20.91248437528 15.0687 14.5265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53955_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53955_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:53:18.81 +19:25:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.166 660670462385900800 133.32819243104 +19.43060751372 14.8382 14.4077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53957_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53957_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53959_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53959_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:39:56.15 +26:54:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.874 703426071543956224 129.98347048967 +26.90889688466 14.7562 14.0255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53963_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53963_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:50:00.88 +22:07:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 0.496 686052825751659520 132.50369627562 +22.12574609630 14.8527 14.1659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53964_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53964_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:50:27.36 +17:52:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 0.636 659940558463692928 132.61395443957 +17.88174530955 14.7529 14.0540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53968_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53968_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:43:21.21 +21:36:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 2.429 664956633588613632 130.83777829336 +21.60472711154 14.7500 14.0213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53976_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53976_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:00:03.96 +26:24:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.951 691753037627545088 135.01602763658 +26.40935558169 14.9608 14.4777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53979_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53979_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:24:10.24 +25:38:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.500 693718998777153280 141.04227124942 +25.63641029251 15.2636 14.8179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53983_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53983_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:48:13.11 +26:18:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.888 691183215727345280 132.05447103790 +26.31614482402 14.7211 13.8484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53986_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53986_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:42:35.20 +19:02:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.169 661026944671335424 130.64644693127 +19.04477734214 14.6263 14.0188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53993_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53993_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:41:24.25 +18:14:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.659 659411796450014464 130.35058468934 +18.23404390253 14.8801 13.8177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.659#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53995_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53995_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:41:38.78 +19:19:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.600 661226574753044224 130.41169300219 +19.33061922441 14.9616 14.4292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53997_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 53997_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:42:05.11 +23:48:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.901 690250108312660480 130.52101200856 +23.80798253316 14.8108 14.3002 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54000_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54000_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:11:29.50 +22:34:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.125 686832620014204544 137.87259201769 +22.57443908107 14.9543 14.4240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54012_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54012_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 09:06:40.68 +18:04:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54013_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
Preparing report for the candidate 54013_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
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Considering the candidate 54022_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54022_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:42:03.17 +17:20:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.297 658534867206917120 130.51284385627 +17.34096246040 14.7937 14.2991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54030_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54030_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:43:48.50 +26:41:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 0.733 703185519013996032 130.95198840705 +26.69960165875 15.0785 14.3621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54047_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54047_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:42:51.41 +24:29:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.331 690314773340136064 130.71442280447 +24.49351920989 14.9112 14.3857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54048_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54048_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:42:15.92 +23:17:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 1.775 666159499310436864 130.56590135572 +23.29420953956 14.7946 13.9457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.775#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54049_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54049_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:53:03.83 +20:01:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 0.900 660840336932288768 133.26585308205 +20.02675727517 14.8399 14.3455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54054_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54054_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:51:09.09 +24:23:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.397 689920151744435584 132.78747691310 +24.38497160095 15.2336 14.7348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54089_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54089_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:42:53.79 +18:55:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 0.402 661010211478828416 130.72422783768 +18.92422320236 14.8490 14.3436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54093_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54093_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:48:16.95 +25:27:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.730 690850849681181312 132.07105778256 +25.45122389915 14.7389 13.9452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54110_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54110_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:43:56.39 +20:08:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 2.193 661384968848577152 130.98431400188 +20.13387349426 14.8231 14.1750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54116_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54116_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:46:46.19 +17:19:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 0.820 658350802088304512 131.69243026997 +17.32891258424 14.7906 14.1746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54123_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 54123_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
**** FOUND 08:48:12.30 +16:54:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 0.494 658274282951142272 132.05138693395 +16.90795762691 14.7751 14.2430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 08312_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122
The candidate 08312_fd_Cnc-03-Q1b1x1_2026-03-22_01-33-20_20.00sec_-15.00C_LIGHT_0122 did not pass the final checks
