This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP
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 27.1777* 10 32 04.12 +05 31 41.3 11.6 U Sex 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,2461098.6777,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.1777 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:32:04.12 +05:31:41.3 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_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 27.1777* 09 53 28.59 +05 15 55.2 12.3 U Sex 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,2461098.6777,12.27,0.05,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 20260227.1777 12.27CV 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:53:28.59 +05:15:55.2 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_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 27.1777* 10 27 39.77 +06 16 54.5 13.2 U Sex 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,2461098.6777,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.1777 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:27:39.77 +06:16:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_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 27.1777* 09 54 11.27 +02 00 17.2 13.4 U Sex 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,2461098.6777,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.1777 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:54:11.27 +02:00:17.2 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_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 27.1777* 10 01 40.04 +03 46 34.8 14.1 U Sex 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,2461098.6777,14.10,0.05,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 20260227.1777 14.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:01:40.04 +03:46:34.8 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_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 27.1777* 10 35 35.89 +06 06 25.4 14.3 U Sex 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,2461098.6777,14.35,0.05,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 20260227.1777 14.35CV 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:35:35.89 +06:06:25.4 ;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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20_00sec_-15_00C_LIGHT_0416_fits__*pix.png resample_wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20_00sec_-14_90C_LIGHT_0152_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: 2461058.87957345 18.01.2026 09:06:25.146 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
First image: 2461058.87957345 18.01.2026 09:06:25.146 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
Last image: 2461098.67802867 27.02.2026 04:16:11.677 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6759
Objects passed selection criteria: 6742
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: 5662.25
Average stars matched: 5575 (98.4591 %)
Memory usage VmPeak: 112984 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 22:21:43 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: 2461058.87957345 18.01.2026 09:06:25.146 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
First image: 2461058.87957345 18.01.2026 09:06:25.146 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
Last image: 2461098.67802867 27.02.2026 04:16:11.677 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 28
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
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: 9 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): 38283
Objects passed selection criteria: 38197
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 34126
Average stars matched: 33289.2 (97.5481 %)
Memory usage VmPeak: 140776 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 22:22:32 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
SExtractor catalog cache: saved Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat to cache
SExtractor catalog cache: saved Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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: 2461098.67741247
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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits exists and is non-empty
Saving wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits to local_wcs_cache/
'wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits' -> 'local_wcs_cache/wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits'
wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits exists and is non-empty
Saving wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits to local_wcs_cache/
'wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits' -> 'local_wcs_cache/wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits'
wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits exists and is non-empty
Saving wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits to local_wcs_cache/
'wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits' -> 'local_wcs_cache/wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits'
wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits exists and is non-empty
Saving wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits to local_wcs_cache/
'wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits' -> 'local_wcs_cache/wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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 10:17:31.152 +06:01:10.35
Second-epoch image center 10:16:59.548 +06:00:05.54
Angular distance between the image centers 0.13 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 10:17:31.152 +06:01:10.35
Second-epoch image center 10:16:57.076 +06:00:31.05
Angular distance between the image centers 0.14 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 10:16:59.548 +06:00:05.54
Second-epoch second image center 10:16:57.076 +06:00:31.05
Angular distance between the image centers 0.01246 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits &> /tmp/tmp.GIconqcYT5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits &> /tmp/tmp.PIuU4vcEPJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits &> /tmp/tmp.LT7FksyRBu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits &> /tmp/tmp.nWt1sXyiqD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits and wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits and wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat
Found non-empty wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits and wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat
The reference image (wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits) and catalog (wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat) found
'wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.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 3983 out of 7065 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.859046
a=0.000000 b=1.000000 c=22.859046
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
2.0 pix Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
2.0 pix fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
2.1 pix fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
Limiting magnitude estimates:
15.3 mag. Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
15.3 mag. Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
14.6 mag. fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
14.6 mag. fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.6 (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.GIconqcYT5 (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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits' -> 'wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
WCS-calibrated image found: wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
Checking if the catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat corresponding to the image wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat corresponding to the image wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
WCS catalog name: wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=518, passed=7065
Got 7065 stars (including 6535 good ones) from the SExtractor catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 7065 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 916 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: 0.31"
Excluding outliers - 916 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits -region wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.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.PIuU4vcEPJ (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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits' -> 'wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
WCS-calibrated image found: wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
Checking if the catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat corresponding to the image wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat corresponding to the image wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
WCS catalog name: wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=518, passed=7072
Got 7072 stars (including 6542 good ones) from the SExtractor catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat
util/solve_plate_with_UCAC5 got 7072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 916 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 916 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: 0.31"
Excluding outliers - 916 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits -region wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.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.LT7FksyRBu (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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
WCS_IMAGE_NAME=wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
WCS-calibrated image found: wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
Checking if the catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat corresponding to the image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat corresponding to the image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
WCS catalog name: wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=393, passed=4328
Got 4328 stars (including 3924 good ones) from the SExtractor catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat
util/solve_plate_with_UCAC5 got 4328 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 920 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 920 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 - 920 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits -region wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.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.nWt1sXyiqD (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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
WCS_IMAGE_NAME=wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
WCS-calibrated image found: wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
Checking if the catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
WCS catalog name: wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=401, passed=4361
Got 4361 stars (including 3957 good ones) from the SExtractor catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat
util/solve_plate_with_UCAC5 got 4361 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 916 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: 0.32"
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 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 915 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits -region wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits'
Saving fully-calibrated image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits'
Preparing the HTML report for the field Sex-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20330.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20330_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
Preparing report for the candidate 20330_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Sex-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 ####
10:32:04.12 +05:31:41.3
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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
SExtractor catalog cache: saved Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat to cache
SExtractor catalog cache: saved Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
Creating symlink local_wcs_cache/wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits exists and is non-empty
wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits exists and is non-empty
wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits exists and is non-empty
wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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 10:17:31.152 +06:01:10.35
Second-epoch image center 10:16:59.548 +06:00:05.54
Angular distance between the image centers 0.13 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 10:17:31.152 +06:01:10.35
Second-epoch image center 10:16:57.076 +06:00:31.05
Angular distance between the image centers 0.14 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 10:16:59.548 +06:00:05.54
Second-epoch second image center 10:16:57.076 +06:00:31.05
Angular distance between the image centers 0.01246 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/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits &> /tmp/tmp.STzet6Lupz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits &> /tmp/tmp.ePTt5N10Tk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits &> /tmp/tmp.WfQ8UDHRbU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits &> /tmp/tmp.b0Pp9c3h7d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits and wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.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_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits and wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat
Found non-empty wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits and wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat
The reference image (wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits) and catalog (wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat) found
'wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.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 4077 out of 40894 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.736338
a=0.000000 b=1.000000 c=22.736338
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
1.9 pix Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
1.9 pix fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
1.9 pix fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
Limiting magnitude estimates:
15.5 mag. Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
15.4 mag. Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
14.8 mag. fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
14.8 mag. fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.2 (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.STzet6Lupz (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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits' -> 'wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
WCS-calibrated image found: wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
Checking if the catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat corresponding to the image wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat corresponding to the image wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits
WCS catalog name: wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1744, passed=40882
Got 40882 stars (including 39070 good ones) from the SExtractor catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 40882 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 912 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: 0.33"
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 912 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: 0.32"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits -region wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-06-25_20.00sec_-15.00C_LIGHT_0416.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.ePTt5N10Tk (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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits' -> 'wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
WCS-calibrated image found: wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
Checking if the catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat corresponding to the image wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat corresponding to the image wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits
WCS catalog name: wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1745, passed=40944
Got 40944 stars (including 39124 good ones) from the SExtractor catalog wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat
util/solve_plate_with_UCAC5 got 40944 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 913 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 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits -region wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-01-Q1b1x1_2026-01-18_03-07-15_20.00sec_-15.00C_LIGHT_0417.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.WfQ8UDHRbU (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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
WCS_IMAGE_NAME=wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
WCS-calibrated image found: wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
Checking if the catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat corresponding to the image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat corresponding to the image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
WCS catalog name: wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=973, passed=27886
Got 27886 stars (including 26858 good ones) from the SExtractor catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat
util/solve_plate_with_UCAC5 got 27886 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 915 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: 0.34"
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 915 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 - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits -region wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.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.b0Pp9c3h7d (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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
WCS_IMAGE_NAME=wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
WCS-calibrated image found: wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
Checking if the catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
WCS catalog name: wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=962, passed=27711
Got 27711 stars (including 26698 good ones) from the SExtractor catalog wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat
util/solve_plate_with_UCAC5 got 27711 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 913 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: 0.34"
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 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits -region wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-15-18_20.00sec_-14.90C_LIGHT_0152.fits
Saving fully-calibrated image wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.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_Sex-01-Q1b1x1_221935_TTUQ1b1x1_26530_BG5A5pfP/wcs_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153.fits
Preparing the HTML report for the field Sex-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53073.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53078.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 52770_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52770_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:47:29.89 +03:47:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52800_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52800_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:32:04.13 +05:31:41.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52807_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52807_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:25:20.46 +08:45:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 0.191 3875926513958932480 156.33529919810 +08.75253403443 11.5522 10.8527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52826_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52826_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:07:40.10 +00:53:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52828_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
Preparing report for the candidate 52828_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
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Considering the candidate 52848_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52848_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:41:28.20 +08:34:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 0.877 3869018484264926592 160.36763929570 +08.57553426313 12.5351 11.9187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52849_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52849_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:42:39.08 +03:33:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 0.526 3857552850024906368 160.66297665660 +03.55922443355 12.5950 12.0853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52853_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52853_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:25:23.30 +08:46:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 0.328 3875926544025225344 156.34715730318 +08.76791551568 12.5539 12.0571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.328#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52899_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
Preparing report for the candidate 52899_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
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Considering the candidate 52908_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
Preparing report for the candidate 52908_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
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Considering the candidate 52939_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52939_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:26:26.81 +05:17:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.461 3860614508872107264 156.61185641271 +05.28640597676 13.7548 13.0721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52952_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52952_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:18:37.39 +07:19:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 0.488 3875352465809799424 154.65584973966 +07.32020609999 13.6184 13.1410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52955_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52955_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:22:15.50 +08:59:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.879 3876004991601317504 155.56490039664 +08.99262465927 13.8168 13.3202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52965_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52965_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:26:12.39 +03:56:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 5.117 3857182722627732736 156.55259813455 +03.95089932231 13.4798 12.7011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52969_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52969_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 09:56:01.48 +07:40:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52979_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52979_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:34:21.06 +02:46:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.270 3856137675480695680 158.58865364239 +02.76726943429 13.5297 12.6499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52996_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 52996_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:29:54.23 +08:02:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 3.567 3863639608957216128 157.47694520695 +08.04002508976 14.0275 13.3777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53006_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 53006_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:18:36.32 +01:34:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.461 3832450243648588800 154.65201262861 +01.57186519147 13.8796 13.3953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53018_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
Preparing report for the candidate 53018_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
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Considering the candidate 53073_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 53073_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:13:20.73 +05:15:33.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)
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Considering the candidate 53078_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
Preparing report for the candidate 53078_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
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Considering the candidate 53087_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 53087_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 10:13:10.46 +04:12:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.438 3860816368044899328 153.29395780618 +04.20238631575 14.3343 13.8411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 02584_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153
The candidate 02584_fd_Sex-01-Q1b1x1_2026-02-26_22-16-11_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks