This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2
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,2461083.7312,12.43,0.05,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 20260212.2312 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:53.51 +18:56:05.1 ;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-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2312* 09 24 30.18 +21 07 02.4 13.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.7312,13.16,0.05,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 20260212.2312 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:24:30.18 +21:07:02.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2312* 09 26 40.06 +22 24 14.6 13.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.7312,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.2312 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:26:40.06 +22:24:14.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2312* 09 22 45.13 +22 40 31.3 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.7312,13.60,0.05,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 20260212.2312 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:22:45.13 +22:40:31.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_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,2461083.7312,13.94,0.05,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 20260212.2312 13.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:47:42.97 +21:58:09.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2312* 09 31 34.60 +20 50 57.2 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461083.7312,14.22,0.05,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 20260212.2312 14.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:31:34.60 +20:50:57.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_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,2461083.7312,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.2312 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:55:30.84 +18:35:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_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,2461083.7312,14.23,0.05,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 20260212.2312 14.23CV 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-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:50:49.96 +20:10:05.7 ;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-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_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,2461083.7312,14.24,0.05,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 20260212.2312 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:21.39 +26:00:07.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_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,2461083.7312,13.29,0.05,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 20260212.2312 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:45.40 +18:48:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20_00sec_-15_00C_LIGHT_0222_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20_00sec_-14_90C_LIGHT_0698_fits__*pix.png resample_wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20_00sec_-14_90C_LIGHT_0221_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
First image: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Last image: 2461083.73149664 12.02.2026 05:33:11.310 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 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): 9060
Objects passed selection criteria: 9048
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: 8562
Average stars matched: 8214.25 (95.9384 %)
Memory usage VmPeak: 117536 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 23:46:27 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: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
First image: 2461033.02376176 23.12.2025 12:34:03.016 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Last image: 2461083.73149664 12.02.2026 05:33:11.310 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 223
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 17 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): 51572
Objects passed selection criteria: 51425
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: 49183.8
Average stars matched: 46569.5 (94.6847 %)
Memory usage VmPeak: 150056 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 23:47:36 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-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.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: 2461083.73095264
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits exists and is non-empty
Saving wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits exists and is non-empty
Saving wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits'
wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.486 +21:59:44.92
Second-epoch image center 09:13:50.733 +22:00:04.91
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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:13:51.065 +21:59:34.64
Angular distance between the image centers 0.00 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:13:50.733 +22:00:04.91
Second-epoch second image center 09:13:51.065 +21:59:34.64
Angular distance between the image centers 0.00851 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits &> /tmp/tmp.dzypNCl1Xx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits &> /tmp/tmp.cbbYhS99iC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits &> /tmp/tmp.cvQ0FFPY84
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.TdQG5Ze3SS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
Found non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
The reference image (wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits) and catalog (wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat) found
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 4769 out of 8632 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.930105
a=0.000000 b=1.000000 c=22.930105
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
2.1 pix Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
1.9 pix fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
2.0 pix fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
Limiting magnitude estimates:
15.3 mag. Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
15.3 mag. Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
15.4 mag. fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
15.4 mag. fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 12.2 (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.dzypNCl1Xx (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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> 'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=673, passed=8632
Got 8632 stars (including 7938 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
util/solve_plate_with_UCAC5 got 8632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits -region wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cbbYhS99iC (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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> 'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=654, passed=8532
Got 8532 stars (including 7867 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
util/solve_plate_with_UCAC5 got 8532 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits -region wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cvQ0FFPY84 (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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=673, passed=8696
Got 8696 stars (including 8019 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 8696 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.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.TdQG5Ze3SS (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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=693, passed=8657
Got 8657 stars (including 7959 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 8657 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.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-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits'
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20655.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20463_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20463_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:19:04.95 +18:19:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20502_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20502_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:51:57.84 +25:43:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20601_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20601_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:45:46.59 +24:47:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20603_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20603_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:43:13.43 +20:13:51.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20618_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20618_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:56:03.02 +16:43:59.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20631_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20631_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:46:46.85 +23:21:57.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20655_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20655_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:33:06.52 +25:03:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.483 645729572536622464 143.27729333734 +25.06270830126 10.8251 9.4285 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20658_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20658_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:30:45.39 +20:14:58.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20660_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20660_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:24:31.84 +22:49:28.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20661_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 20661_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:26:33.72 +24:12:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01624_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 01624_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:09:52.62 +25:14:53.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits exists and is non-empty
wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.486 +21:59:44.92
Second-epoch image center 09:13:50.733 +22:00:04.91
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 09:13:50.486 +21:59:44.92
Second-epoch image center 09:13:51.065 +21:59:34.64
Angular distance between the image centers 0.00 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:13:50.733 +22:00:04.91
Second-epoch second image center 09:13:51.065 +21:59:34.64
Angular distance between the image centers 0.00851 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits &> /tmp/tmp.dnwLRirKHQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits &> /tmp/tmp.sqysQzAa4O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits &> /tmp/tmp.Pwq5Y2v0aH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits &> /tmp/tmp.vVPAoy8hxH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
Found non-empty wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits and wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
The reference image (wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits) and catalog (wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat) found
'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 4825 out of 48025 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.818215
a=0.000000 b=1.000000 c=22.818215
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 56 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
2.0 pix Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
1.8 pix fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
1.8 pix fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
Limiting magnitude estimates:
15.5 mag. Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
15.4 mag. Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
15.5 mag. fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
15.5 mag. fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
All-image limiting magnitude estimate: 15.5 (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.dnwLRirKHQ (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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits' -> 'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
SExtractor catalog parsing summary: zero_flux=11, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2316, passed=47999
Got 47999 stars (including 45610 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat
util/solve_plate_with_UCAC5 got 47999 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits -region wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-03_20.00sec_-14.90C_LIGHT_0698.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.sqysQzAa4O (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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits' -> 'wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat corresponding to the image wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=2292, passed=48027
Got 48027 stars (including 45647 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat
util/solve_plate_with_UCAC5 got 48027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits -region wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2025-12-23_06-34-40_20.00sec_-14.90C_LIGHT_0699.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Pwq5Y2v0aH (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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=2548, passed=50876
Got 50876 stars (including 48230 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat
util/solve_plate_with_UCAC5 got 50876 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.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.vVPAoy8hxH (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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=2615, passed=51095
Got 51095 stars (including 48379 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 51095 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cnc-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.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-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-32-24_20.00sec_-14.90C_LIGHT_0221.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.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-03-Q1b1x1_234211_TTUQ1b1x1_2596_Luofc8G2/wcs_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222.fits
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out54299.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out40690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53698.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53824.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54208.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54252.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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: 7s
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Considering the candidate 53458_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53458_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:43:13.21 +17:07:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53461_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53461_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:48:05.49 +18:51:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.126 660285354141566848 132.02319590224 +18.85193583124 14.6311 14.1900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53464_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53464_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:46:24.86 +19:43:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53467_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53467_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:46:18.95 +26:21:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53468_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53468_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:45:25.92 +20:25:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.951 661768771422658816 131.35814915334 +20.42288681745 14.1476 13.2198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53469_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53469_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:55:27.58 +18:31:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53473_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53473_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:38:27.21 +20:38:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53475_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53475_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:48:38.00 +20:14:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53478_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53478_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:10:18.93 +20:32:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53483_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53483_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:43:56.55 +22:33:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53527_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53527_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:51:57.81 +25:43:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53628_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53628_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:45:46.59 +24:47:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53643_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53643_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:56:03.03 +16:43:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53698_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
Preparing report for the candidate 53698_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
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Considering the candidate 53726_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53726_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:01:20.44 +22:31:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53731_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53731_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:47:05.30 +26:45:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53798_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53798_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:13:27.98 +25:25:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.192 688540264650971392 138.36662931568 +25.41750571804 12.9637 12.4960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.192#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53824_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
Preparing report for the candidate 53824_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
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Considering the candidate 53832_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53832_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:41:43.77 +19:16:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53888_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
Preparing report for the candidate 53888_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
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Considering the candidate 53896_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53896_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:47:26.13 +26:53:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.428 647130870041690624 146.85881318771 +26.89057747287 13.3645 12.9178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53939_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
Preparing report for the candidate 53939_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
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Considering the candidate 53964_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53964_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:55:10.27 +26:15:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53998_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 53998_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:47:06.47 +26:42:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.423 646740990090406912 146.77689547302 +26.70251972847 13.7774 13.3931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54015_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54015_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:58:18.27 +22:50:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54047_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54047_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:53:41.24 +20:38:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.109 661651432915840384 133.42164495043 +20.64828042404 14.0066 13.4947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54067_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
Preparing report for the candidate 54067_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
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Considering the candidate 54068_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54068_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:38:35.91 +19:25:42.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54072_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54072_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:44:01.65 +25:18:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54083_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54083_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:29:04.47 +17:51:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54100_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54100_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:28:03.04 +25:56:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54152_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54152_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:31:11.61 +21:09:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.964 634858804152156928 142.79890587499 +21.15684036404 14.0129 13.2245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54181_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
Preparing report for the candidate 54181_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
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Considering the candidate 54191_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54191_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:51:20.67 +17:21:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54195_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54195_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:43:35.01 +20:50:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.134 661843813091122176 130.89645192798 +20.83971865387 14.2658 13.6518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54208_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
Preparing report for the candidate 54208_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
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Considering the candidate 54210_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54210_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:54:31.90 +22:50:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54227_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54227_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:45:28.07 +19:22:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54232_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54232_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:46:08.50 +19:14:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.273 661071337453244160 131.53568580450 +19.24388479235 14.4128 13.9956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54236_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54236_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:50:00.96 +19:18:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54251_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
Preparing report for the candidate 54251_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
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Considering the candidate 54252_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
Preparing report for the candidate 54252_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
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Considering the candidate 54256_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54256_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:17:52.15 +25:59:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54260_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54260_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:38:19.62 +17:28:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.125 620867694782646400 144.58128553153 +17.47744561267 14.6227 13.9566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54276_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54276_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:50:40.44 +23:41:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54287_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54287_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:33:55.78 +26:48:37.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54293_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54293_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:47:11.96 +23:43:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.816 689544634163804160 131.80013627249 +23.71937041078 14.6395 14.1708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54299_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54299_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:43:08.22 +21:10:57.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)
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Considering the candidate 54307_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54307_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:43:23.14 +20:36:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54346_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54346_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:44:51.23 +20:52:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54359_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54359_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:46:57.41 +18:35:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54364_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 54364_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 08:44:37.48 +25:02:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.497 690634903022325248 131.15626326891 +25.03544873371 14.5658 14.0473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.497#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 02553_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 02553_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:46:17.03 +26:20:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08312_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 08312_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks
**** FOUND 09:09:52.62 +25:14:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02562_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222
The candidate 02562_fd_Cnc-03-Q1b1x1_2026-02-11_23-33-11_20.00sec_-15.00C_LIGHT_0222 did not pass the final checks