This analysis is done by the script util/transients/transient_factory_test31.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461049.6388,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260109.1388 12.51CV 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:32:07.81 +03:52:38.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 09.1388* 02 13 20.27 +06 24 17.7 13.5 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461049.6388,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260109.1388 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:13:20.27 +06:24:17.7 ;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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 01 09.1388* 02 07 21.54 +04 30 11.7 13.9 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461049.6388,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260109.1388 13.91CV 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:21.54 +04:30:11.7 ;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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_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,2461049.6388,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260109.1388 14.20CV 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:17:16.26 +08:43:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_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,2461049.6388,14.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260109.1388 14.49CV 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 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:55:10.72 +09:22:01.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20_00sec_-14_90C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20_00sec_-15_00C_LIGHT_0164_fits__*pix.png resample_wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20_00sec_-15_00C_LIGHT_0091_fits__*pix.png animation_v2.gif
Processing complete!
Total number of candidates identified: 5
Processing log:
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.67881661 23.12.2025 04:17:19.755 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
First image: 2461032.67881661 23.12.2025 04:17:19.755 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
Last image: 2461049.63905728 09.01.2026 03:20:04.549 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
Estimated ref. image limiting mag.: -10.52
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: 1
User-specified moving object: none
Computation time: 22 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 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): 6966
Objects passed selection criteria: 6964
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 6742.5
Average stars matched: 6632 (98.3611 %)
Memory usage VmPeak: 109804 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Thu Jan 8 15:05:04 -00 2026
VaST build number 1.0rc88-133-gdb8b9ae6
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jan 9 04:17:14 -00 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.67881661 23.12.2025 04:17:19.755 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
First image: 2461032.67881661 23.12.2025 04:17:19.755 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
Last image: 2461049.63905728 09.01.2026 03:20:04.549 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 56
Estimated ref. image limiting mag.: -7.95
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: 1
User-specified moving object: none
Computation time: 72 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 2.1 # or , in mag.arcsec-2
ANALYSIS_THRESH 2.1 # or , in mag.arcsec-2
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): 35633
Objects passed selection criteria: 35552
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 34651.2
Average stars matched: 33414.2 (96.4301 %)
Memory usage VmPeak: 133516 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Thu Jan 8 15:05:04 -00 2026
VaST build number 1.0rc88-133-gdb8b9ae6
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Jan 9 04:21:49 -00 2026
Host name: tau
############################################################
Filtering log:
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst
CAMERA_SETTINGS= TTUQ1b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR= /var/www/nmw_calibration/TTUQ1b1x1/darks
EXCLUSION_LIST= ../exclusion_list_TTUQ1.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE= /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
FRAME_EDGE_OFFSET_PIX= 50
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= no
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 1
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
Reference image directory is set to /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved/
VIZIER_SITE=vizier.cds.unistra.fr
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Psc-06-Q1b1x1
#######################################
########### Starting Psc-06-Q1b1x1 ###########
Processing Psc-06-Q1b1x1
server tau has sufficient free disk space available: 596789 MB at /mnt/usb2/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 596789 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
REFERENCE_EPOCH__SECOND_IMAGE= /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.png' -> 'transient_report/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits_preview.png'
Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
renamed 'Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.png' -> 'transient_report/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits_preview.png'
Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 637.4324
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 529.8526
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1156.1238
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 561.5628
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1157.8756
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 560.3448
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.81372
INFO: SECOND_EPOCH__SD_ratio= 0.002
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR=/var/www/nmw_calibration/TTUQ1b1x1/darks FLAT_FIELD_FILE=/var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -15.0 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2026-01-08T21:19:19.5185525' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-09T03:19:19.5185525' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61049.1384203471 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-09T03:19:29.4209025' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61049.1385349538 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -15.0 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 25.7117689495437 / [deg] RA of telescope" status=0
Record 32: "DEC = 6.00011698123627 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 50.4502777777778 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 232.603611111111 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.29599145431195 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Psc-06' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '01 42 51' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+06 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/d_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits :)
Spent 0.532146 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/d_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -14.9 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2026-01-08T21:20:04.5499665' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-09T03:20:04.5499665' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61049.1389415395 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-09T03:20:14.4528556' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61049.1390561573 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -14.9 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 25.7117689894742 / [deg] RA of telescope" status=0
Record 32: "DEC = 6.00011699683633 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 50.3233333333333 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 232.8275 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.29836303966055 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Psc-06' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '01 42 51' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+06 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
CCD-TEMP= -14.900000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/d_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits :)
Spent 0.666894 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/d_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Dark frame used to calibrate the second-epoch images:
Flat field used to calibrate the second-epoch images:
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Previews of the CALIBRATED second-epoch images:
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 1 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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: 2461049.63853609
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits exists and is non-empty
Saving wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits to local_wcs_cache/
'wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits' -> 'local_wcs_cache/wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits'
wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits exists and is non-empty
Saving wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits to local_wcs_cache/
'wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits' -> 'local_wcs_cache/wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits'
wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits exists and is non-empty
Saving wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits to local_wcs_cache/
'wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits' -> 'local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits'
wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits exists and is non-empty
Saving wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits to local_wcs_cache/
'wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits' -> 'local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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 01:42:40.430 +05:58:40.48
Second-epoch image center 01:42:52.022 +05:59:59.07
Angular distance between the image centers 0.05 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 01:42:40.430 +05:58:40.48
Second-epoch image center 01:42:54.435 +05:59:18.86
Angular distance between the image centers 0.06 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits &> /tmp/tmp.s52aYA1btT
Parallel run for /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits &> /tmp/tmp.hSH1Si5eUp
Parallel run for /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits &> /tmp/tmp.TVwKghCdr4
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits &> /tmp/tmp.NomvMQWjJ1
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits and wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits and wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat
Found non-empty wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits and wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat
The reference image (wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits) and catalog (wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat) found
'wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.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 3826 out of 7028 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.925555
a=0.000000 b=1.000000 c=22.925555
From vast_summary.log: estimated ref. image limiting mag.: -10.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 12.41
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 12.41
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
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:
2.1 pix Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
2.1 pix Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
2.0 pix fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
2.0 pix fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
All-image limiting magnitude estimate: 12.2 with default.sex.telephoto_lens_onlybrightstars_v1
(80th percentile of magnitude distribution of stars detected on all four images)
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.s52aYA1btT (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits 573.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
verification OK: /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits' -> 'wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits'
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
DEBUG: WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat corresponding to the image wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat corresponding to the image wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=480, passed=7028
Got 7028 stars (including 6537 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat
util/solve_plate_with_UCAC5 got 7028 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
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: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
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: 0.24"
Estimated accuracy of the plate solution: 0.21"
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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits -region wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.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.hSH1Si5eUp (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits 573.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
verification OK: /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits' -> 'wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits'
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
DEBUG: WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat corresponding to the image wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat corresponding to the image wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=486, passed=6953
Got 6953 stars (including 6453 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat
util/solve_plate_with_UCAC5 got 6953 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
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: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.25"
ITERATION 02 -- talking to VizieR, this might be slow!
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: 0.25"
Estimated accuracy of the plate solution: 0.22"
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_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits -region wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.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.TVwKghCdr4 (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits 605.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
DEBUG: WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=496, passed=6612
Got 6612 stars (including 6108 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 6612 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
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: 0.29"
Estimated accuracy of the plate solution: 0.26"
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_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -region wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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.NomvMQWjJ1 (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits 605.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
DEBUG: WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=499, passed=6549
Got 6549 stars (including 6045 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat
util/solve_plate_with_UCAC5 got 6549 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
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_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -region wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
'wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.fz' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.fz'
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
'wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.fz' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.fz'
Preparing the HTML report for the field Psc-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20276.dat to exclusion_list_gaiadr2.txt
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20267_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
The candidate 20267_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092 did not pass the final checks
**** FOUND 01:59:10.27 +07:34:48.4 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.35 -c=01:59:10.27 +07:34:48.4 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 0.418 2568076639813043456 029.79267457942 +07.58011473152 12.4890 11.8839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
Prepared the HTML report for the field Psc-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 1 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
Creating symlink local_wcs_cache/wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Creating symlink local_wcs_cache/exclusion_list_bsc.txt
Creating symlink local_wcs_cache/exclusion_list_tycho2.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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits exists and is non-empty
wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits exists and is non-empty
wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits exists and is non-empty
wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.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 01:42:40.430 +05:58:40.48
Second-epoch image center 01:42:52.022 +05:59:59.07
Angular distance between the image centers 0.05 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 01:42:40.430 +05:58:40.48
Second-epoch image center 01:42:54.435 +05:59:18.86
Angular distance between the image centers 0.06 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits &> /tmp/tmp.LKNQrhcWAH
Parallel run for /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits &> /tmp/tmp.SPTbtyPCj8
Parallel run for /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits &> /tmp/tmp.eLZ8c7Y7Wc
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits &> /tmp/tmp.rmDVQTvvm4
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits and wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits and wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat
Found non-empty wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits and wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat
The reference image (wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits) and catalog (wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat) found
'wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.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 3883 out of 34515 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.827577
a=0.000000 b=1.000000 c=22.827577
From vast_summary.log: estimated ref. image limiting mag.: -7.95
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.88
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.88
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
2.0 pix Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
1.9 pix fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
1.9 pix fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
All-image limiting magnitude estimate: 14.7 with default.sex.telephoto_lens_vSTL
(80th percentile of magnitude distribution of stars detected on all four images)
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.LKNQrhcWAH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits 573.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
verification OK: /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits' -> 'wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits'
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
DEBUG: WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat corresponding to the image wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat corresponding to the image wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1452, passed=34509
Got 34509 stars (including 32998 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat
util/solve_plate_with_UCAC5 got 34509 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 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: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.23"
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_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits -region wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.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.SPTbtyPCj8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits 573.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
verification OK: /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits' -> 'wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits'
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
DEBUG: WCS_IMAGE_NAME=wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
WCS-calibrated image found: wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
Checking if the catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat corresponding to the image wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits alredy exist and is non-empty...
Catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat corresponding to the image wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits
WCS catalog name: wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1468, passed=34996
Got 34996 stars (including 33471 good ones) from the SExtractor catalog wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat
util/solve_plate_with_UCAC5 got 34996 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
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: 0.27"
Estimated accuracy of the plate solution: 0.23"
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_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/2025-12-22/LIGHT/calibrated_platesolved//Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits -region wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-06-Q1b1x1_2025-12-22_22-18-11_20.00sec_-15.00C_LIGHT_0165.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.eLZ8c7Y7Wc (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits 605.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
DEBUG: WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1455, passed=34890
Got 34890 stars (including 33385 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 34890 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
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: 0.31"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits -region wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.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.rmDVQTvvm4 (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits 605.0
Entering WCS image calibration mode.
DEBUG: ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
DEBUG: FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
DEBUG: FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
DEBUG: WCS_IMAGE_NAME=wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS-calibrated image found: wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
Checking if the catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
WCS catalog name: wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1476, passed=35038
Got 35038 stars (including 33495 good ones) from the SExtractor catalog wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat
util/solve_plate_with_UCAC5 got 35038 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.28"
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_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits -region wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.fits.fz
Saving fully-calibrated image wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-08_CI_Psc-06-Q1b1x1_220315_TTUQ1b1x1_24931_sGuDKlZ2/wcs_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.fits.fz
Preparing the HTML report for the field Psc-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52642.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52704.dat to exclusion_list_local.txt
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Considering the candidate 52537_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
The candidate 52537_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092 did not pass the final checks
**** FOUND 02:10:08.42 +10:43:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52545_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
The candidate 52545_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092 did not pass the final checks
**** FOUND 01:44:06.91 +02:48:50.4 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..13.26 -c=01:44:06.91 +02:48:50.4 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 1.596 2512298204482583808 026.02875180601 +02.81444156848 12.3869 11.7743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52575_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
Preparing report for the candidate 52575_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
Successfully moved Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.png to transient_report/52575_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_reference.png
Successfully moved Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.png to transient_report/Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits_preview.png
Successfully moved fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.png to transient_report/52575_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_discovery1.png
Successfully moved fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.png to transient_report/52575_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_discovery2.png
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Considering the candidate 52600_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
The candidate 52600_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092 did not pass the final checks
**** FOUND 01:21:32.94 +09:14:08.9 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..14.41 -c=01:21:32.94 +09:14:08.9 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 1.028 2579163530951954816 020.38705765651 +09.23601877464 13.4887 12.8668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52617_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
Preparing report for the candidate 52617_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
Successfully moved Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.png to transient_report/52617_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_reference.png
The output file transient_report/Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits_preview.png already exist
Successfully moved fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.png to transient_report/52617_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_discovery1.png
Successfully moved fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.png to transient_report/52617_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_discovery2.png
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Considering the candidate 52642_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
Preparing report for the candidate 52642_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
Successfully moved Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.png to transient_report/52642_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_reference.png
The output file transient_report/Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits_preview.png already exist
Successfully moved fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.png to transient_report/52642_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_discovery1.png
Successfully moved fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.png to transient_report/52642_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_discovery2.png
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Considering the candidate 52648_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
The candidate 52648_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092 did not pass the final checks
**** FOUND 01:31:14.78 +08:48:52.8 in Gaia DR2 single (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06, VIZIER_COMMAND=#lib/vizquery -site=vizier.cds.unistra.fr -mime=text -source=I/345/gaia2 -out.max=3 -out.add=_r -out.form=mini -sort=Gmag Gmag=0.0..15.06 -c=01:31:14.78 +08:48:52.8 -c.rs=14.75 -out=Source,RA_ICRS,DE_ICRS,Gmag,RPmag,Var#)VIZIER_GAIADR2_OUTPUT=# 1.765 2566951186582773248 022.81166261698 +08.81515054862 14.2501 13.6872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52674_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
Preparing report for the candidate 52674_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
Successfully moved Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.png to transient_report/52674_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_reference.png
The output file transient_report/Psc-06-Q1b1x1_2025-12-22_22-17-19_20.00sec_-15.00C_LIGHT_0164.fits_preview.png already exist
Successfully moved fd_Psc-06-Q1b1x1_2026-01-08_21-19-19_20.00sec_-15.00C_LIGHT_0091.png to transient_report/52674_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_discovery1.png
Successfully moved fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092.png to transient_report/52674_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092_discovery2.png
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Considering the candidate 52697_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092
The candidate 52697_fd_Psc-06-Q1b1x1_2026-01-08_21-20-04_20.00sec_-14.90C_LIGHT_0092 did not pass the final checks
