This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.1497* 02 11 31.53 +06 56 26.1 12.9 U Cet 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,2461083.6497,12.95,0.05,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 20260212.1497 12.95CV 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:11:31.53 +06:56:26.1 ;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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_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 12.1497* 02 30 16.82 +05 55 50.0 13.3 U Cet 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,2461083.6497,13.26,0.05,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 20260212.1497 13.26CV 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:30:16.82 +05:55:50.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_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 12.1497* 02 34 16.82 +10 20 24.4 13.8 U Cet 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,2461083.6497,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.1497 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:34:16.82 +10:20:24.4 ;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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_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 12.1497* 02 33 53.91 +09 12 44.4 14.4 U Cet 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,2461083.6497,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260212.1497 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:33:53.91 +09:12:44.4 ;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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_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 12.1497* 03 01 34.16 +07 39 50.8 14.4 U Cet 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,2461083.6497,14.45,0.05,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 20260212.1497 14.45CV 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:01:34.16 +07:39:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20_00sec_-15_00C_LIGHT_0100_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20_00sec_-14_90C_LIGHT_0099_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.70779689 23.12.2025 04:59:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
First image: 2461032.70779689 23.12.2025 04:59:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Last image: 2461083.64996065 12.02.2026 03:35:46.600 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
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): 6713
Objects passed selection criteria: 6710
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: 6334.75
Average stars matched: 6239.5 (98.4964 %)
Memory usage VmPeak: 112992 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 21:40:28 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.70779689 23.12.2025 04:59:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
First image: 2461032.70779689 23.12.2025 04:59:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Last image: 2461083.64996065 12.02.2026 03:35:46.600 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 36
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 10 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): 35988
Objects passed selection criteria: 35906
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: 34819
Average stars matched: 33848.2 (97.212 %)
Memory usage VmPeak: 137552 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 21:41:19 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
SExtractor catalog cache: saved Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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: 2461083.64949819
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits exists and is non-empty
Saving wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits to local_wcs_cache/
'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits' -> 'local_wcs_cache/wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits'
wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
Saving wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits to local_wcs_cache/
'wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits' -> 'local_wcs_cache/wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits'
wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
Saving wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits to local_wcs_cache/
'wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits' -> 'local_wcs_cache/wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits'
wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits exists and is non-empty
Saving wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits to local_wcs_cache/
'wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits' -> 'local_wcs_cache/wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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 02:34:05.473 +05:59:28.46
Second-epoch image center 02:34:18.682 +05:58:35.81
Angular distance between the image centers 0.06 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 02:34:05.473 +05:59:28.46
Second-epoch image center 02:34:17.933 +05:59:00.36
Angular distance between the image centers 0.05 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 02:34:18.682 +05:58:35.81
Second-epoch second image center 02:34:17.933 +05:59:00.36
Angular distance between the image centers 0.00749 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits &> /tmp/tmp.OOtQXdE7j7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.OOthDw9ePP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits &> /tmp/tmp.zCD5JW9mkK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits &> /tmp/tmp.7TInpbJmoD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
Found non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
The reference image (wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits) and catalog (wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat) found
'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.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 3725 out of 7100 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.925639
a=0.000000 b=1.000000 c=22.925639
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
2.1 pix Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
2.0 pix fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
2.0 pix fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
Limiting magnitude estimates:
15.3 mag. Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
15.3 mag. Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
15.1 mag. fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
15.1 mag. fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.0 (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.OOtQXdE7j7 (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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits' -> 'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Checking if the catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS catalog name: wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=484, passed=7100
Got 7100 stars (including 6611 good ones) from the SExtractor catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 7100 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits -region wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.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.OOthDw9ePP (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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=486, passed=7027
Got 7027 stars (including 6535 good ones) from the SExtractor catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 7027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.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.zCD5JW9mkK (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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=432, passed=5694
Got 5694 stars (including 5252 good ones) from the SExtractor catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 5694 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 969 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: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 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: 0.31"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits -region wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.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.7TInpbJmoD (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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=433, passed=5646
Got 5646 stars (including 5206 good ones) from the SExtractor catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 5646 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 970 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: 0.35"
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 970 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: 0.33"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits -region wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits'
Saving fully-calibrated image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits'
Preparing the HTML report for the field Cet-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cet-01-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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
SExtractor catalog cache: saved Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Creating symlink local_wcs_cache/wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits exists and is non-empty
wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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 02:34:05.473 +05:59:28.46
Second-epoch image center 02:34:18.682 +05:58:35.81
Angular distance between the image centers 0.06 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 02:34:05.473 +05:59:28.46
Second-epoch image center 02:34:17.933 +05:59:00.36
Angular distance between the image centers 0.05 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 02:34:18.682 +05:58:35.81
Second-epoch second image center 02:34:17.933 +05:59:00.36
Angular distance between the image centers 0.00749 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/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits &> /tmp/tmp.359ljHGZ1E
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.SLluHK4Ho7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits &> /tmp/tmp.2ihRCQ8UYJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits &> /tmp/tmp.FhPN3cw5kB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
Found non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
The reference image (wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits) and catalog (wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat) found
'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.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 3771 out of 36889 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.832485
a=0.000000 b=1.000000 c=22.832485
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 19 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
2.0 pix Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
1.9 pix fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
1.9 pix fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
Limiting magnitude estimates:
15.5 mag. Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
15.5 mag. Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
15.2 mag. fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
15.2 mag. fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (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.359ljHGZ1E (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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits' -> 'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Checking if the catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS catalog name: wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1585, passed=36879
Got 36879 stars (including 35234 good ones) from the SExtractor catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 36879 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits -region wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.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.SLluHK4Ho7 (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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1594, passed=37071
Got 37071 stars (including 35410 good ones) from the SExtractor catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 37071 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.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.2ihRCQ8UYJ (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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1225, passed=33063
Got 33063 stars (including 31777 good ones) from the SExtractor catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 33063 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 968 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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits -region wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.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.FhPN3cw5kB (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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1200, passed=33088
Got 33088 stars (including 31817 good ones) from the SExtractor catalog wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 33088 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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 968 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: 0.36"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits -region wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-06_20.00sec_-14.90C_LIGHT_0099.fits
Saving fully-calibrated image wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.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_Cet-01-Q1b1x1_213815_TTUQ1b1x1_32348_08wXi1mG/wcs_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100.fits
Preparing the HTML report for the field Cet-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52747.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 52556_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52556_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:33:45.67 +08:24:58.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)
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Considering the candidate 52558_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52558_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:37:00.35 +02:16:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52559_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52559_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:05:56.30 +07:31:59.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 52609_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 52609_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 52621_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52621_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:38:03.42 +02:02:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.604 2502287705162424448 039.51386298727 +02.03700098945 13.2699 12.6265 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52628_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 52628_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 52629_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52629_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:46:50.29 +01:58:41.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52637_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52637_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:56:08.77 +08:21:40.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52658_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52658_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:42:32.29 +06:14:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.617 18596766010620800 040.63435316049 +06.23826926927 13.6539 12.9738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52665_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52665_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:25:44.19 +10:31:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52675_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 52675_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 52685_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52685_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:13:11.70 +04:45:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52691_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52691_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:26:48.78 +03:44:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.458 2515685804102694016 036.70333212903 +03.74812509694 13.7313 13.1926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52706_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52706_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:15:13.71 +05:30:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52731_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 52731_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 52747_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 52747_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 52769_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52769_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:04:32.46 +10:22:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 3.981 2571106928218918528 031.13423269575 +10.38099851964 14.6907 14.1166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52792_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 52792_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 02:41:21.27 +05:03:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 2.058 6028008075336576 040.33848885553 +05.06163854061 14.6128 14.0538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07540_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100
The candidate 07540_fd_Cet-01-Q1b1x1_2026-02-11_21-35-46_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks