This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461082.7466,9.18,0.05,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 20260211.2466 9.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:17.05 +20:08:07.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,12.07,0.05,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 20260211.2466 12.07CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:55:27.45 +19:49:45.8 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,12.23,0.05,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 20260211.2466 12.23CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:52:27.73 +24:05:01.4 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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
target,2461082.7466,14.37,0.05,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
target 20260211.2466 14.37CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:22:44.82 +24:17:46.8 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,12.85,0.05,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 20260211.2466 12.85CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:18.84 +25:40:52.8 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,13.06,0.05,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 20260211.2466 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:47:53.07 +25:35:40.2 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2466 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:03:04.36 +20:34:00.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,13.71,0.05,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 20260211.2466 13.71CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:02:38.01 +23:07:25.5 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,13.80,0.05,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 20260211.2466 13.80CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:34.12 +21:56:59.4 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,14.10,0.05,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 20260211.2466 14.10CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:47:13.91 +24:40:01.5 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,14.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.2466 14.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:27:35.37 +25:42:42.3 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,14.32,0.05,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 20260211.2466 14.32CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:49:11.72 +25:55:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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,2461082.7466,14.41,0.05,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 20260211.2466 14.41CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:39:47.97 +22:27:06.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_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
GV Cnc,2461082.7466,12.25,0.05,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
GV Cnc 20260211.2466 12.25CV 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:27:40.54 +19:15:43.9 ;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-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20_00sec_-15_00C_LIGHT_0224_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20_00sec_-15_00C_LIGHT_0510_fits__*pix.png resample_wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20_00sec_-15_00C_LIGHT_0223_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.90559659 23.12.2025 09:43:53.545 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
First image: 2461032.90559659 23.12.2025 09:43:53.545 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Last image: 2461082.74696345 11.02.2026 05:55:27.642 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 4 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): 14570
Objects passed selection criteria: 14561
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: 14152.5
Average stars matched: 13851.5 (97.8732 %)
Memory usage VmPeak: 119212 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 00:03:38 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.90559659 23.12.2025 09:43:53.545 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
First image: 2461032.90559659 23.12.2025 09:43:53.545 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Last image: 2461082.74696345 11.02.2026 05:55:27.642 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 281
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 34 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): 83779
Objects passed selection criteria: 83576
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 80667.5
Average stars matched: 78212.8 (96.957 %)
Memory usage VmPeak: 1878196 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 00:05:17 CST 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.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: 2461082.74629737
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits exists and is non-empty
Saving wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits to local_wcs_cache/
'wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits'
wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits exists and is non-empty
Saving wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits to local_wcs_cache/
'wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits' -> 'local_wcs_cache/wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits'
wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits'
wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits exists and is non-empty
Saving wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits to local_wcs_cache/
'wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits' -> 'local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:28.113 +21:59:58.59
Second-epoch image center 08:18:27.321 +22:00:20.59
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.113 +21:59:58.59
Second-epoch image center 08:18:24.979 +22:00:21.80
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:18:27.321 +22:00:20.59
Second-epoch second image center 08:18:24.979 +22:00:21.80
Angular distance between the image centers 0.00905 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits &> /tmp/tmp.UtAPaWh4Cn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits &> /tmp/tmp.JuSEq5Z2ds
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits &> /tmp/tmp.BHhTloYkvt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits &> /tmp/tmp.wF276wkXvf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
Found non-empty wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
The reference image (wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits) and catalog (wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat) found
'wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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 7184 out of 14630 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.976505
a=0.000000 b=1.000000 c=22.976505
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
2.1 pix Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
2.5 pix fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
2.5 pix fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
Limiting magnitude estimates:
15.5 mag. Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
15.5 mag. Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
15.3 mag. fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
15.3 mag. fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.UtAPaWh4Cn (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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits' -> 'wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1109, passed=14630
Got 14630 stars (including 13511 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
util/solve_plate_with_UCAC5 got 14630 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits -region wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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.JuSEq5Z2ds (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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits' -> 'wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1116, passed=14643
Got 14643 stars (including 13509 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat
util/solve_plate_with_UCAC5 got 14643 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits -region wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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.BHhTloYkvt (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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1152, passed=13873
Got 13873 stars (including 12704 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat
util/solve_plate_with_UCAC5 got 13873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.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.wF276wkXvf (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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1118, passed=13793
Got 13793 stars (including 12660 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat
util/solve_plate_with_UCAC5 got 13793 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 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.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_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits'
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits'
Preparing the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20830.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20850.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 20823_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20823_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:49:53.78 +21:26:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20829_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20829_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:08:29.57 +17:13:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20830_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 20830_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20840_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20840_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:48:57.64 +18:11:08.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20847_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20847_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:45:16.58 +21:29:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20848_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 20848_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20849_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20849_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:27:40.54 +19:15:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.755 662945695541783296 126.91869458160 +19.26220098895 11.2080 9.8317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.755#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20850_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 20850_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20851_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20851_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:25:42.25 +25:43:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20852_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20852_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:53:20.92 +18:40:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20855_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20855_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:16:38.47 +22:55:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.766 677297960119209216 124.16015441056 +22.92652336314 12.3459 12.1625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20858_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20858_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:46:53.72 +25:10:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 0.626 690816391160130048 131.72365544232 +25.17249000915 12.4579 11.9986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20859_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 20859_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:18:26.67 +21:40:45.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05338_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 05338_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:11:03.22 +23:08:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11161_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 11161_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:35:46.23 +18:53:45.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10707_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 10707_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:53:43.44 +19:16:23.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:05:17.05 +20:08:07.0
07:55:27.45 +19:49:45.8
07:52:27.73 +24:05:01.4
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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat to cache
SExtractor catalog cache: saved Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Creating symlink local_wcs_cache/wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits exists and is non-empty
wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits exists and is non-empty
wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:18:28.113 +21:59:58.59
Second-epoch image center 08:18:27.321 +22:00:20.59
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:18:28.113 +21:59:58.59
Second-epoch image center 08:18:24.979 +22:00:21.80
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:18:27.321 +22:00:20.59
Second-epoch second image center 08:18:24.979 +22:00:21.80
Angular distance between the image centers 0.00905 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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits &> /tmp/tmp.rMulvKpVzw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits &> /tmp/tmp.NFecqv2nKf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits &> /tmp/tmp.Dv0AOSb3xs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits &> /tmp/tmp.DiMq0uD1mK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
Found non-empty wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits and wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
The reference image (wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits) and catalog (wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat) found
'wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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 7219 out of 84420 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.884013
a=0.000000 b=1.000000 c=22.884013
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.59
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.59
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 82 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
2.0 pix Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
2.3 pix fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
2.3 pix fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
Limiting magnitude estimates:
15.6 mag. Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
15.6 mag. Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
15.4 mag. fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
15.4 mag. fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rMulvKpVzw (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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits' -> 'wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=5639, passed=84389
Got 84389 stars (including 78614 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat
util/solve_plate_with_UCAC5 got 84389 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits -region wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-43-53_20.00sec_-15.00C_LIGHT_0510.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.NFecqv2nKf (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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits' -> 'wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS_IMAGE_NAME=wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS-calibrated image found: wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
Checking if the catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits alredy exist and is non-empty...
Catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat corresponding to the image wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits
WCS catalog name: wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=5720, passed=84301
Got 84301 stars (including 78450 good ones) from the SExtractor catalog wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat
util/solve_plate_with_UCAC5 got 84301 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits -region wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-02-Q1b1x1_2025-12-23_03-44-37_20.00sec_-14.90C_LIGHT_0511.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.Dv0AOSb3xs (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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=6293, passed=78100
Got 78100 stars (including 71677 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat
util/solve_plate_with_UCAC5 got 78100 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 975 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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.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.DiMq0uD1mK (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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
WCS-calibrated image found: wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
Checking if the catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat corresponding to the image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
WCS catalog name: wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=6271, passed=78076
Got 78076 stars (including 71672 good ones) from the SExtractor catalog wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat
util/solve_plate_with_UCAC5 got 78076 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 974 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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits -region wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.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_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-54-30_20.00sec_-15.00C_LIGHT_0223.fits
Saving fully-calibrated image wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.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_2026-02-11_CI_Cnc-02-Q1b1x1_000236_TTUQ1b1x1_18428_mXwfLE2y/wcs_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224.fits
Preparing the HTML report for the field Cnc-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out100601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100606.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100644.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100654.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out100811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out100598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100741.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100771.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75548.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 6s
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Considering the candidate 100589_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100589_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:58:54.34 +24:08:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100598_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100598_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100599_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100599_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:49:47.45 +20:18:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100601_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100601_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:38:54.91 +21:00:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.295 664526724542399104 129.72814846282 +21.00328621339 14.5093 14.1046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100606_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100606_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:08:51.74 +26:10:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.577 683439492771015296 122.21496106247 +26.17830896960 14.1917 13.5462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100608_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100608_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:05:51.66 +20:04:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 2.038 670519440871002624 121.46537517300 +20.08110934443 14.4791 13.9196 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100609_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100609_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:04:11.07 +19:10:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100614_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100614_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:47:52.64 +24:48:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100615_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100615_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:52:44.04 +25:43:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100616_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100616_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:46:35.35 +25:43:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100617_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100617_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:56:02.48 +18:41:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100619_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100619_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:46:59.31 +24:39:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100621_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100621_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:47:03.50 +20:41:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100622_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100622_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 100625_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100625_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:21:13.61 +16:58:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100628_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100628_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:10:53.53 +17:12:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100632_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100632_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:48:12.98 +26:04:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100633_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100633_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:46:43.68 +21:58:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100636_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100636_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:09:12.22 +19:27:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.349 669675806215201536 122.30065630592 +19.45767215326 13.9533 13.4857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100637_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100637_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:51:57.58 +20:18:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100638_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100638_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:56:22.61 +24:35:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100639_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100639_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:05:31.46 +25:08:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100641_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100641_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:50:26.16 +24:50:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100642_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100642_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:40:15.95 +22:27:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.119 665259033646251520 130.06593587595 +22.45514229048 13.9666 13.4486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100643_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100643_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:36:42.69 +18:53:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100644_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100644_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:48:52.96 +25:41:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.865 874005301910270208 117.22019907832 +25.69724563912 13.7285 13.2403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100645_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100645_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:47:18.94 +19:55:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100648_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100648_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:09:27.67 +18:37:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100654_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100654_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:53:38.34 +23:38:42.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 100655_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100655_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:02:59.76 +18:02:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100656_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100656_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:57:56.82 +18:50:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.746 669992774801454976 119.48678685116 +18.84848209292 12.9379 12.2367 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100657_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100657_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:53:22.61 +17:17:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100658_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100658_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:00:09.64 +24:15:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100659_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100659_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:53:07.51 +23:37:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100661_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100661_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:45:31.58 +23:25:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100663_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100663_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:59:05.21 +19:11:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100664_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100664_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:49:53.79 +21:26:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100665_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100665_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:00:25.55 +21:36:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100666_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100666_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:33:16.67 +18:20:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100668_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100668_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:08:29.57 +17:13:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100669_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100669_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:57:12.44 +23:40:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100671_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100671_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:05:17.04 +20:08:06.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 100685_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100685_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:45:16.57 +21:29:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100686_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100686_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:55:27.50 +19:49:45.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 100687_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100687_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:52:27.74 +24:05:01.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 100692_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100692_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:53:07.30 +18:58:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100698_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100698_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100705_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100705_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100706_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100706_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:01:15.86 +19:30:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100712_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100712_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100714_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100714_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:55:06.57 +21:27:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100716_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100716_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:13:02.79 +17:59:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100718_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100718_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:55:47.15 +18:16:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100719_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100719_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:59:27.81 +16:55:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100726_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100726_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:14:21.15 +17:05:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100728_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100728_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:43:51.43 +18:22:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100732_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100732_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100733_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100733_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:55:44.86 +22:42:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100738_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100738_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:38:42.41 +16:55:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 3.036 658460306574666880 129.67582698162 +16.92328189531 14.0348 13.5525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100740_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100740_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:57:07.36 +17:20:05.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100741_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100741_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100744_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100744_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:07:02.84 +17:09:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100748_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100748_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:56:57.07 +19:55:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100757_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100757_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:48:21.90 +18:11:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100764_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100764_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:58:14.61 +18:28:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100767_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100767_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:49:39.95 +18:46:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100771_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100771_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100781_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100781_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:52:40.38 +25:53:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.229 873837935624124672 118.16769034895 +25.88872313848 14.5335 14.1009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 100783_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100783_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:54:15.20 +20:31:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100787_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100787_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:53:46.13 +18:03:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100793_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100793_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100795_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100795_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:51:05.28 +18:43:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100799_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100799_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100805_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100805_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:59:13.38 +20:40:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100809_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100809_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:56:06.72 +19:12:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 100811_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100811_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 07:51:27.57 +17:43:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.406 668321070451885696 117.86426110470 +17.72257334224 14.6091 14.1145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100813_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
Preparing report for the candidate 100813_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
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Considering the candidate 100831_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 100831_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:12:23.87 +17:15:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73108_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 73108_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:35:46.23 +18:53:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31007_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 31007_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
**** FOUND 08:11:03.22 +23:08:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75057_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224
The candidate 75057_fd_Cnc-02-Q1b1x1_2026-02-10_23-55-27_20.00sec_-15.00C_LIGHT_0224 did not pass the final checks
