This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 02 32 19.11 +08 30 56.3 13.0 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,2461098.6218,13.01,0.05,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 20260227.1218 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:32:19.11 +08:30:56.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 02 45 26.48 +07 46 12.1 13.2 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,2461098.6218,13.21,0.05,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 20260227.1218 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:45:26.48 +07:46:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 02 07 10.91 +01 09 59.2 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
target,2461098.6218,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.1218 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:07:10.91 +01:09:59.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 03 04 23.71 +07 39 38.8 14.2 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
target,2461098.6218,14.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.1218 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:04:23.71 +07:39:38.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 02 59 36.52 +10 53 32.1 14.3 U Ari 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
target,2461098.6218,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.1218 14.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:59:36.52 +10:53:32.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1218* 03 00 30.02 +08 57 51.4 14.3 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.6218,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.1218 14.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:00:30.02 +08:57:51.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20_00sec_-15_00C_LIGHT_0064_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png resample_wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20_00sec_-15_00C_LIGHT_0063_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.70779689 23.12.2025 04:59:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
First image: 2461032.70779689 23.12.2025 04:59:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Last image: 2461098.62202622 27.02.2026 02:55:33.065 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 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): 6677
Objects passed selection criteria: 6652
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 5347.25
Average stars matched: 5256 (98.2935 %)
Memory usage VmPeak: 112996 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 26 20:58:49 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.70779689 23.12.2025 04:59:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
First image: 2461032.70779689 23.12.2025 04:59:03.651 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Last image: 2461098.62202622 27.02.2026 02:55:33.065 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 106
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 34610
Objects passed selection criteria: 34524
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 29807.8
Average stars matched: 29013.5 (97.3354 %)
Memory usage VmPeak: 137552 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 26 20:59:36 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
SExtractor catalog cache: saved Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.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: 2461098.62160360
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_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits exists and is non-empty
Saving wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits to local_wcs_cache/
'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits' -> 'local_wcs_cache/wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits'
wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
Saving wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits to local_wcs_cache/
'wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits' -> 'local_wcs_cache/wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits'
wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits exists and is non-empty
Saving wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits to local_wcs_cache/
'wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits' -> 'local_wcs_cache/wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits'
wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits exists and is non-empty
Saving wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits to local_wcs_cache/
'wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits' -> 'local_wcs_cache/wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:34:05.473 +05:59:28.46
Second-epoch image center 02:34:25.456 +05:59:40.37
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:34:05.473 +05:59:28.46
Second-epoch image center 02:34:24.908 +05:59:44.63
Angular distance between the image centers 0.08 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 02:34:25.456 +05:59:40.37
Second-epoch second image center 02:34:24.908 +05:59:44.63
Angular distance between the image centers 0.00256 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits &> /tmp/tmp.Oth4JNKkud
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.raMrjdRr2t
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits &> /tmp/tmp.apgvmket5K
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits &> /tmp/tmp.83w1pK6Ki1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
Found non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
The reference image (wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits) and catalog (wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat) found
'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3725 out of 7100 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.925639
a=0.000000 b=1.000000 c=22.925639
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
2.1 pix Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
2.1 pix fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
2.0 pix fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
Limiting magnitude estimates:
15.3 mag. Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
15.3 mag. Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
14.4 mag. fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
14.4 mag. fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Oth4JNKkud (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits' -> 'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Checking if the catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS catalog name: wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=484, passed=7100
Got 7100 stars (including 6611 good ones) from the SExtractor catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 7100 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits -region wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.raMrjdRr2t (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=486, passed=7027
Got 7027 stars (including 6535 good ones) from the SExtractor catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 7027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.apgvmket5K (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=330, passed=3692
Got 3692 stars (including 3358 good ones) from the SExtractor catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 3692 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 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: 0.29"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits -region wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.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.83w1pK6Ki1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=349, passed=3682
Got 3682 stars (including 3323 good ones) from the SExtractor catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 3682 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits -region wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits'
Saving fully-calibrated image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits'
Preparing the HTML report for the field Cet-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cet-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
SExtractor catalog cache: saved Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat to cache
SExtractor catalog cache: saved Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Creating symlink local_wcs_cache/wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits exists and is non-empty
wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits exists and is non-empty
wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits exists and is non-empty
wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:34:05.473 +05:59:28.46
Second-epoch image center 02:34:25.456 +05:59:40.37
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:34:05.473 +05:59:28.46
Second-epoch image center 02:34:24.908 +05:59:44.63
Angular distance between the image centers 0.08 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 02:34:25.456 +05:59:40.37
Second-epoch second image center 02:34:24.908 +05:59:44.63
Angular distance between the image centers 0.00256 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits &> /tmp/tmp.EQcoQX0Yff
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits &> /tmp/tmp.WUkNPfvhmv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits &> /tmp/tmp.1414Lb6rPS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits &> /tmp/tmp.YBccT6vm8e
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
Found non-empty wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits and wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
The reference image (wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits) and catalog (wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat) found
'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3771 out of 36889 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.832485
a=0.000000 b=1.000000 c=22.832485
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 91 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
2.0 pix Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
2.0 pix fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
1.9 pix fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
Limiting magnitude estimates:
15.5 mag. Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
15.5 mag. Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
14.6 mag. fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
14.6 mag. fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.EQcoQX0Yff (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits' -> 'wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS-calibrated image found: wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
Checking if the catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits
WCS catalog name: wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1585, passed=36879
Got 36879 stars (including 35234 good ones) from the SExtractor catalog wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 36879 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits -region wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-01-Q1b1x1_2025-12-22_22-59-03_20.00sec_-14.90C_LIGHT_0208.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WUkNPfvhmv (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits' -> 'wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
Checking if the catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat corresponding to the image wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits
WCS catalog name: wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1594, passed=37071
Got 37071 stars (including 35410 good ones) from the SExtractor catalog wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 37071 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits -region wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-01-Q1b1x1_2025-12-22_23-00-07_20.00sec_-14.90C_LIGHT_0209.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1414Lb6rPS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
Checking if the catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
WCS catalog name: wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=867, passed=23139
Got 23139 stars (including 22230 good ones) from the SExtractor catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 23139 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits -region wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.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.YBccT6vm8e (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
WCS-calibrated image found: wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
Checking if the catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat corresponding to the image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
WCS catalog name: wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=825, passed=22926
Got 22926 stars (including 22055 good ones) from the SExtractor catalog wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 22926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits -region wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-54-56_20.00sec_-15.00C_LIGHT_0063.fits
Saving fully-calibrated image wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Cet-01-Q1b1x1_205624_TTUQ1b1x1_5971_15TsljPl/wcs_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064.fits
Preparing the HTML report for the field Cet-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53047.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 52589_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52589_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52590_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52590_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 52593_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52593_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52598_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52598_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52602_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52602_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52603_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52603_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52608_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52608_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52612_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
Preparing report for the candidate 52612_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
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Considering the candidate 52615_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52615_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52616_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52616_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52617_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52617_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52618_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52618_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
**** FOUND 02:09:35.60 +04:13:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.177 2518134313418534400 032.39774311132 +04.22572283380 13.0592 12.6110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52619_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52619_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52622_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52622_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 52623_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52623_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52626_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52626_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52627_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52627_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52633_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52633_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52635_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
Preparing report for the candidate 52635_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
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Considering the candidate 52637_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52637_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52641_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52641_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52645_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52645_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
**** FOUND 02:46:50.18 +01:58:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52662_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52662_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52666_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52666_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
**** FOUND 02:56:08.65 +08:21:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52669_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52669_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 52671_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52671_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52685_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52685_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52687_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52687_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 52689_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52689_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52690_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52690_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
**** FOUND 02:37:13.14 +02:25:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52692_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52692_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52695_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52695_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52716_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52716_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52728_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52728_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52731_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52731_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52732_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52732_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
**** FOUND 02:59:36.76 +08:53:41.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52740_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52740_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52741_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52741_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
**** FOUND 02:22:15.54 +02:28:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52743_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52743_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 52749_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52749_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52753_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52753_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52760_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52760_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 52763_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52763_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 52765_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52765_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52778_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52778_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 52784_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52784_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52785_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52785_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
**** FOUND 02:25:44.20 +10:31:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52802_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52802_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52807_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52807_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52810_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52810_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 52825_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52825_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52845_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52845_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 52846_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52846_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52860_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52860_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 52873_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52873_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 52878_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
Preparing report for the candidate 52878_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
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Considering the candidate 52880_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52880_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 52885_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52885_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 52894_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52894_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52896_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52896_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52921_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52921_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 52946_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52946_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52948_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52948_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 52965_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
Preparing report for the candidate 52965_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
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Considering the candidate 52966_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52966_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 52970_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52970_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 52977_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52977_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 52999_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 52999_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 53000_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53000_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 53007_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53007_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 53013_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53013_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 53027_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
Preparing report for the candidate 53027_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
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Considering the candidate 53028_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53028_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 53029_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53029_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 53034_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53034_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 53035_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53035_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53037_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53037_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 53040_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53040_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53046_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53046_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 53047_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
Preparing report for the candidate 53047_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
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Considering the candidate 53048_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53048_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 53050_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53050_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 53052_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53052_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 53055_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53055_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 53058_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53058_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 53061_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53061_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 53064_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53064_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 53071_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53071_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 53075_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53075_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 53078_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53078_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 53086_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064
The candidate 53086_fd_Cet-01-Q1b1x1_2026-02-26_20-55-33_20.00sec_-15.00C_LIGHT_0064 did not pass the final checks