This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.8173,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.3173 12.08CV 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/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:06:44.08 -10:33:56.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V3745 Oph,2461125.8173,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V3745 Oph 20260326.3173 12.69CV 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/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:32:33.24 -13:04:07.9 ;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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.8173,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.3173 13.35CV 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/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:14:47.63 -09:11:38.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.8173,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.3173 13.29CV 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/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:49:41.72 -12:43:29.4 ;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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.8173,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.3173 13.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:24:48.74 -10:05:58.3 ;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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0718 Oph,2461125.8173,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0718 Oph 20260326.3173 13.22CV 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/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:31:36.53 -07:41:04.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20_00sec_-10_00C_LIGHT_0581_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20_00sec_-10_00C_LIGHT_0580_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: 2461098.96964103 27.02.2026 11:16:06.985 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
First image: 2461098.96964103 27.02.2026 11:16:06.985 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
Last image: 2461125.81768779 26.03.2026 07:37:18.225 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.82
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: 4 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): 6420
Objects passed selection criteria: 6409
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: 5585.75
Average stars matched: 5507 (98.5902 %)
Memory usage VmPeak: 112928 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 02:47:55 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.96964103 27.02.2026 11:16:06.985 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
First image: 2461098.96964103 27.02.2026 11:16:06.985 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
Last image: 2461125.81768779 26.03.2026 07:37:18.225 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 42
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 21 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): 51372
Objects passed selection criteria: 51276
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: 45818.2
Average stars matched: 44546.8 (97.2249 %)
Memory usage VmPeak: 154956 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 02:48:51 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
SExtractor catalog cache: saved Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.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/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.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: 2461125.81700750
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits'
wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits'
wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits'
wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits exists and is non-empty
Saving wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits to local_wcs_cache/
'wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits' -> 'local_wcs_cache/wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.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 16:17:09.506 -09:59:57.78
Second-epoch image center 16:17:09.637 -10:00:12.36
Angular distance between the image centers 0.00 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 16:17:09.506 -09:59:57.78
Second-epoch image center 16:17:12.767 -09:59:38.57
Angular distance between the image centers 0.01 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 16:17:09.637 -10:00:12.36
Second-epoch second image center 16:17:12.767 -09:59:38.57
Angular distance between the image centers 0.01591 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/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits &> /tmp/tmp.TALUxr4LDN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.lahO0OIGM9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits &> /tmp/tmp.yf9sGcGRuG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits &> /tmp/tmp.vT6KG700iD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat
Found non-empty wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat
The reference image (wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits) and catalog (wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat) found
'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.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 4172 out of 7717 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.904854
a=0.000000 b=1.000000 c=22.904854
From vast_summary.log: estimated ref. image limiting mag.: -7.82
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.08
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.08
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
2.0 pix Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
2.4 pix fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
2.4 pix fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Limiting magnitude estimates:
15.1 mag. Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
15.1 mag. Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
14.5 mag. fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
14.5 mag. fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
All-image limiting magnitude estimate: 14.5 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.TALUxr4LDN (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits' -> 'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
Checking if the catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
WCS catalog name: wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=484, passed=7717
Got 7717 stars (including 7219 good ones) from the SExtractor catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 7717 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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits -region wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.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.lahO0OIGM9 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits' -> 'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=451, passed=7719
Got 7719 stars (including 7254 good ones) from the SExtractor catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 7719 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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.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.yf9sGcGRuG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
Checking if the catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
WCS catalog name: wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=287, passed=5101
Got 5101 stars (including 4812 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat
util/solve_plate_with_UCAC5 got 5101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits -region wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.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.vT6KG700iD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Checking if the catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS catalog name: wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=289, passed=5066
Got 5066 stars (including 4773 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat
util/solve_plate_with_UCAC5 got 5066 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits -region wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits'
Saving fully-calibrated image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits'
Saving fully-calibrated image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits'
Saving fully-calibrated image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits'
Preparing the HTML report for the field Sco-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03951_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 03951_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:26:52.41 -09:49:54.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06845_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 06845_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:39:42.82 -05:46:28.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Sco-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
SExtractor catalog cache: saved Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits exists and is non-empty
wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits exists and is non-empty
wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.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 16:17:09.506 -09:59:57.78
Second-epoch image center 16:17:09.637 -10:00:12.36
Angular distance between the image centers 0.00 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 16:17:09.506 -09:59:57.78
Second-epoch image center 16:17:12.767 -09:59:38.57
Angular distance between the image centers 0.01 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 16:17:09.637 -10:00:12.36
Second-epoch second image center 16:17:12.767 -09:59:38.57
Angular distance between the image centers 0.01591 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/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits &> /tmp/tmp.Igbqo0490G
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.hhB67TzfCF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits &> /tmp/tmp.NNfYECNHbb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits &> /tmp/tmp.okAB4xCGkD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat
Found non-empty wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat
The reference image (wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits) and catalog (wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat) found
'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.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 4296 out of 62618 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.769220
a=0.000000 b=1.000000 c=22.769220
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
1.9 pix Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
2.2 pix fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
2.1 pix fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Limiting magnitude estimates:
15.3 mag. Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
15.2 mag. Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
14.6 mag. fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
14.7 mag. fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Igbqo0490G (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits' -> 'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
Checking if the catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
WCS catalog name: wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2805, passed=62606
Got 62606 stars (including 59699 good ones) from the SExtractor catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 62606 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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits -region wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.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.hhB67TzfCF (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits' -> 'wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2730, passed=62432
Got 62432 stars (including 59601 good ones) from the SExtractor catalog wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 62432 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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 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 - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.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.NNfYECNHbb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
Checking if the catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
WCS catalog name: wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1622, passed=39796
Got 39796 stars (including 38129 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat
util/solve_plate_with_UCAC5 got 39796 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits -region wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.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.okAB4xCGkD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS_IMAGE_NAME=wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS-calibrated image found: wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Checking if the catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat corresponding to the image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
WCS catalog name: wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1580, passed=40543
Got 40543 stars (including 38912 good ones) from the SExtractor catalog wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat
util/solve_plate_with_UCAC5 got 40543 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010422 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits -region wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.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_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/wcs_Sco-01-Q2b1x1_2026-02-27_05-16-06_20.00sec_-15.00C_LIGHT_0018.fits
Saving fully-calibrated image wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/wcs_Sco-01-Q2b1x1_2026-02-27_05-16-42_20.00sec_-14.90C_LIGHT_0019.fits
Saving fully-calibrated image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-36-19_20.00sec_-10.00C_LIGHT_0580.fits
Saving fully-calibrated image wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Sco-01-Q2b1x1_024451_TTUQ2b1x1_8630_bAoBeqYb/wcs_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581.fits
Preparing the HTML report for the field Sco-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out77360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77385.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out58073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77460.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: 5s
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Considering the candidate 77360_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77360_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:22:34.75 -10:10:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 1.229 4344376707150560768 245.64449514151 -10.17129533636 14.2928 13.6348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.229#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77364_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77364_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:14:48.92 -09:06:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.747 4345309264809744896 243.70387088327 -09.10774017875 14.0849 13.4223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77366_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77366_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:30:29.01 -08:28:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.406 4350707110987947136 247.62097992548 -08.48001643533 14.3217 13.5791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77368_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77368_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:14:33.34 -12:45:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 1.304 4342074879558297856 243.63854530524 -12.76180548429 14.0814 13.4213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77375_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77375_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:32:32.84 -06:58:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 0.702 4351435193843520640 248.13694864405 -06.96717560851 13.7611 12.9437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77379_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77379_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 15:58:41.13 -09:15:55.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)
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Considering the candidate 77380_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77380_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:35:52.52 -06:19:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.283 4351581428889220992 248.96876433923 -06.33215616419 13.6933 13.0327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77383_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77383_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:32:06.36 -06:46:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.815 4351453370145283584 248.02626240739 -06.76674897145 13.6051 12.8624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77385_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77385_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:25:49.75 -08:18:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.542 4350856369690911488 246.45743198990 -08.31447461018 13.9140 13.2804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77387_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77387_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:40:07.98 -06:35:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.241 4352813088070887808 250.03290412532 -06.59972321057 13.7008 13.0140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77388_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77388_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:38:59.16 -07:07:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 0.832 4351241404918367744 249.74633719885 -07.13027932611 13.3809 12.5190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77390_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77390_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:38:27.24 -11:27:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.571 4331055024269336704 249.61364578675 -11.45879122902 13.0106 12.0563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77392_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77392_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:22:43.90 -12:34:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 0.720 4331435077333710336 245.68279302243 -12.56709050377 13.3478 12.5356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77393_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77393_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:27:48.67 -08:41:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.768 4350772600648603904 246.95264147118 -08.69070803453 13.1251 12.5495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77396_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77396_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 15:50:08.41 -13:34:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.355 6263929876729742080 237.53490892591 -13.57478531059 12.8733 12.3041 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77398_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77398_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:29:48.38 -10:12:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77399_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77399_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:31:46.36 -12:26:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77410_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
Preparing report for the candidate 77410_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
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Considering the candidate 77414_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
Preparing report for the candidate 77414_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
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Considering the candidate 77427_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
Preparing report for the candidate 77427_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
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Considering the candidate 77429_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
Preparing report for the candidate 77429_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
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Considering the candidate 77436_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77436_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:37:29.44 -11:51:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77455_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77455_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:15:45.00 -08:22:32.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 77460_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
Preparing report for the candidate 77460_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
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Considering the candidate 77462_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77462_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:28:33.46 -08:14:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.916 4350825411566845440 247.13958811592 -08.24214376764 13.9768 13.1876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77492_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77492_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:37:55.38 -05:58:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 1.930 4353093394816489216 249.48053073102 -05.97568422716 14.4618 13.6891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77503_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 77503_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:18:30.39 -11:11:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.58, MAG_FAINT_SEARCH_LIMIT=15.56)GAIADR2_OUTPUT=# 0.619 4343835403832445568 244.62660744526 -11.18502345383 14.7678 14.0858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32505_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 32505_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks
**** FOUND 16:26:52.39 -09:49:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46081_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581
The candidate 46081_fd_Sco-01-Q2b1x1_2026-03-26_02-37-18_20.00sec_-10.00C_LIGHT_0581 did not pass the final checks