This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BQ Cep,2461126.8149,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
BQ Cep 20260327.3149 11.21CV 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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:26:55.71 +68:25:11.0 ;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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0608 Cep,2461126.8149,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
V0608 Cep 20260327.3149 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 21:55:34.30 +67:08:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.8149,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260327.3149 12.38CV 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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:30:22.98 +70:24:52.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2048268+670502,2461126.8149,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
NSVS J2048268+670502 20260327.3149 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:48:27.20 +67:05:00.4 ;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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2218262+670550,2461126.8149,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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
NSVS J2218262+670550 20260327.3149 12.11CV 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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:18:26.23 +67:05:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20_00sec_-15_00C_LIGHT_0310_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20_00sec_-15_00C_LIGHT_0026_fits__*pix.png resample_wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20_00sec_-14_90C_LIGHT_0309_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: 2461036.55907558 27.12.2025 01:24:54.130 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
First image: 2461036.55907558 27.12.2025 01:24:54.130 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Last image: 2461126.81607027 27.03.2026 07:34:58.471 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.89
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): 12904
Objects passed selection criteria: 12831
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 8419.5
Average stars matched: 8047.25 (95.5787 %)
Memory usage VmPeak: 118368 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 02:37:08 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55907558 27.12.2025 01:24:54.130 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
First image: 2461036.55907558 27.12.2025 01:24:54.130 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Last image: 2461126.81607027 27.03.2026 07:34:58.471 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 37
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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: 14 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): 83023
Objects passed selection criteria: 82790
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 54845.5
Average stars matched: 51866 (94.5675 %)
Memory usage VmPeak: 1920000 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 02:38:20 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat to cache
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.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: 2461126.81373588
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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits exists and is non-empty
Saving wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits to local_wcs_cache/
'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits' -> 'local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits'
wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits exists and is non-empty
Saving wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits to local_wcs_cache/
'wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits' -> 'local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits'
wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits exists and is non-empty
Saving wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits to local_wcs_cache/
'wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits' -> 'local_wcs_cache/wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits'
wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits exists and is non-empty
Saving wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits to local_wcs_cache/
'wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits' -> 'local_wcs_cache/wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.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 21:36:17.803 +69:59:41.29
Second-epoch image center 21:36:06.611 +69:58:57.24
Angular distance between the image centers 0.02 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 21:36:17.803 +69:59:41.29
Second-epoch image center 21:36:09.317 +69:58:21.29
Angular distance between the image centers 0.03 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 21:36:06.611 +69:58:57.24
Second-epoch second image center 21:36:09.317 +69:58:21.29
Angular distance between the image centers 0.01071 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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits &> /tmp/tmp.hrHPGki6ik
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits &> /tmp/tmp.ac5SY8imOY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits &> /tmp/tmp.Jl8idyTLZI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits &> /tmp/tmp.u2M5OSDh3P
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
The reference image (wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits) and catalog (wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat) found
'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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 8864 out of 14757 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.917528
a=0.000000 b=1.000000 c=22.917528
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
2.4 pix Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
3.8 pix fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
3.0 pix fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
Limiting magnitude estimates:
15.0 mag. Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
15.0 mag. Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
13.3 mag. fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
13.4 mag. fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 10.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hrHPGki6ik (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1317, passed=14757
Got 14757 stars (including 13425 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 14757 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 973 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits -region wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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.ac5SY8imOY (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1330, passed=14774
Got 14774 stars (including 13430 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 14774 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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits -region wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.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.Jl8idyTLZI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
WCS_IMAGE_NAME=wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
WCS-calibrated image found: wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
Checking if the catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
WCS catalog name: wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=139, passed=4422
Got 4422 stars (including 4283 good ones) from the SExtractor catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat
util/solve_plate_with_UCAC5 got 4422 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 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 964 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: 0.79"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.80"
Estimated accuracy of the plate solution: 0.80"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits -region wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.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.u2M5OSDh3P (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
WCS_IMAGE_NAME=wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
WCS-calibrated image found: wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
Checking if the catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
WCS catalog name: wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=169, passed=4565
Got 4565 stars (including 4394 good ones) from the SExtractor catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat
util/solve_plate_with_UCAC5 got 4565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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: 0.66"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits -region wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits'
Saving fully-calibrated image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits'
Saving fully-calibrated image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits'
Saving fully-calibrated image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits'
Preparing the HTML report for the field Cep-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21043_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 21043_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 20:29:33.49 +67:02:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04404_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 04404_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:41:56.23 +71:18:41.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05514_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 05514_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:28:40.07 +70:33:38.1 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cep-04-Q2b1x1 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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat to cache
SExtractor catalog cache: saved Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Creating symlink local_wcs_cache/wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
Creating symlink local_wcs_cache/wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits exists and is non-empty
wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits exists and is non-empty
wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits exists and is non-empty
wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.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 21:36:17.803 +69:59:41.29
Second-epoch image center 21:36:06.611 +69:58:57.24
Angular distance between the image centers 0.02 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 21:36:17.803 +69:59:41.29
Second-epoch image center 21:36:09.317 +69:58:21.29
Angular distance between the image centers 0.03 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 21:36:06.611 +69:58:57.24
Second-epoch second image center 21:36:09.317 +69:58:21.29
Angular distance between the image centers 0.01071 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/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits &> /tmp/tmp.liUzmby7lt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits &> /tmp/tmp.pdO4Qdw6n3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits &> /tmp/tmp.bhZzPI8Xno
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits &> /tmp/tmp.IjQlNnIJKy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
Calibrating the magnitude scale
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
Found non-empty wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits and wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
The reference image (wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits) and catalog (wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat) found
'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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 9231 out of 98064 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.759782
a=0.000000 b=1.000000 c=22.759782
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.19
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
2.2 pix Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
3.9 pix fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
3.0 pix fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
Limiting magnitude estimates:
15.2 mag. Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
15.2 mag. Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
13.3 mag. fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
13.5 mag. fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 12.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.liUzmby7lt (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=9697, passed=98031
Got 98031 stars (including 88176 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat
util/solve_plate_with_UCAC5 got 98031 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 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.42"
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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits -region wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.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.pdO4Qdw6n3 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits' -> 'wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS_IMAGE_NAME=wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS-calibrated image found: wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Checking if the catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits alredy exist and is non-empty...
Catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat corresponding to the image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
WCS catalog name: wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=9846, passed=98099
Got 98099 stars (including 88083 good ones) from the SExtractor catalog wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat
util/solve_plate_with_UCAC5 got 98099 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 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: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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: 0.42"
Estimated accuracy of the plate solution: 0.42"
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_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits -region wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.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.bhZzPI8Xno (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
WCS_IMAGE_NAME=wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
WCS-calibrated image found: wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
Checking if the catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
WCS catalog name: wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=967, passed=21982
Got 21982 stars (including 21003 good ones) from the SExtractor catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat
util/solve_plate_with_UCAC5 got 21982 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010427 (37.5 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 961 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: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits -region wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.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.IjQlNnIJKy (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
WCS_IMAGE_NAME=wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
WCS-calibrated image found: wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
Checking if the catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits alredy exist and is non-empty...
Catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat corresponding to the image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
WCS catalog name: wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1020, passed=27378
Got 27378 stars (including 26330 good ones) from the SExtractor catalog wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat
util/solve_plate_with_UCAC5 got 27378 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010428 (37.5 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 963 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.66"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits -region wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.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_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/wcs_Cep-04-Q2b1x1_2025-12-26_19-24-54_20.00sec_-15.00C_LIGHT_0026.fits
Saving fully-calibrated image wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/wcs_Cep-04-Q2b1x1_2025-12-26_19-25-35_20.00sec_-15.00C_LIGHT_0027.fits
Saving fully-calibrated image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-31-36_20.00sec_-14.90C_LIGHT_0309.fits
Saving fully-calibrated image wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Cep-04-Q2b1x1_023548_TTUQ2b1x1_10785_qSvvhffo/wcs_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310.fits
Preparing the HTML report for the field Cep-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out28274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90213.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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: 2s
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Considering the candidate 116871_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 116871_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:28:06.12 +70:34:10.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 116914_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 116914_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 22:09:42.08 +72:18:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117493_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 117493_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 22:12:27.53 +73:19:24.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117704_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 117704_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:57:31.64 +66:09:49.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117862_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 117862_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 20:49:41.76 +72:15:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118141_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 118141_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 22:24:38.14 +71:01:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118162_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 118162_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 22:12:55.08 +69:00:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118311_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 118311_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:06:39.54 +71:27:09.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118370_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 118370_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 22:33:26.52 +70:21:05.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118464_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 118464_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:59:19.79 +73:08:50.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118474_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 118474_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:49:19.26 +66:48:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118793_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 118793_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:25:25.37 +70:27:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119141_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 119141_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 20:44:09.85 +67:20:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85158_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 85158_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 20:29:33.57 +67:02:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12421_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 12421_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 22:28:14.86 +72:42:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53023_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 53023_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 22:08:26.61 +68:18:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45855_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
Preparing report for the candidate 45855_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
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Considering the candidate 90213_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
Preparing report for the candidate 90213_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
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Considering the candidate 94801_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 94801_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:40:08.73 +68:02:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28274_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
Preparing report for the candidate 28274_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
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Considering the candidate 94776_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 94776_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 20:36:39.01 +68:17:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71131_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
Preparing report for the candidate 71131_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
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Considering the candidate 108701_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 108701_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:02:07.39 +73:25:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64661_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
Preparing report for the candidate 64661_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
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Considering the candidate 36031_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 36031_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:28:40.06 +70:33:38.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 28861_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 28861_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:41:56.26 +71:18:41.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21503_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 21503_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:43:04.03 +72:19:09.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33833_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 33833_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 22:10:37.97 +70:07:56.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 83027_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 83027_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:27:46.29 +66:48:34.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 17407_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 17407_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 22:09:48.55 +72:20:25.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 13022_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 13022_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks
**** FOUND 21:59:14.66 +73:10:42.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 25378_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310
The candidate 25378_fd_Cep-04-Q2b1x1_2026-03-27_02-34-58_20.00sec_-15.00C_LIGHT_0310 did not pass the final checks